JP6387986B2 - Optical telescope observation plan creation support device and system - Google Patents

Description

  The present invention relates to an apparatus and system that assists in creating an optical telescope observation plan for observing artificial satellites, debris, and the like around the earth with an optical telescope.

  In order to observe artificial satellites and debris in outer space with an optical telescope installed on the ground, it is necessary that the direction of the observation object is not obstructed by clouds or the like. In the prior art, it has been proposed to use a weather forecast value to determine whether or not an observation object can be observed, and to make an observation plan based on the determination.

Japanese Patent No. 5200736

"Special Materials for the 6th" Space Debris Workshop "Lecture Collection", Japan Aerospace Exploration Agency, Japan Aerospace Exploration Agency, March 2015, p.554

  The weather forecast value does not necessarily indicate the actual weather situation of the installation location of the optical telescope and the sky above it. Not only is the weather model incomplete, but the spatial and temporal resolution of forecast values is a major problem. In the mountains, which are considered to be suitable places for the installation of optical telescopes, the weather conditions are easily affected by local topography, and change both spatially and temporally. The weather forecast value does not necessarily satisfy the resolution that represents the weather condition at the point. Whether or not observation in the direction in which the observation object exists is possible should be determined based on whether or not there is a cloud in that direction, that is, the cloud distribution. When the spatial resolution of weather forecast values is low, there is a problem that one forecast value at a low altitude occupies a wide range of the field of view looking up from the telescope installation location. In these respects, the weather forecast value is insufficient data for determining whether or not debris can be observed with an optical telescope. An observation plan designed based on weather forecast values does not use an optical telescope sufficiently efficiently.

  The present invention has been made to solve the above-described problems, and makes it easy to grasp the actual situation over the place where the optical telescope is installed, and efficiently uses artificial satellites and debris with the optical telescope. The purpose is to assist the operator in creating a plan for observation.

An observation plan creation support apparatus for an optical telescope according to the present invention includes a telescope data storage unit for storing telescope data including an installation location of an optical telescope and maximum observable range data which is data for determining a maximum observable range of the optical telescope; the optical telescope predicted trajectory and the predicted orbit storage unit for storing for each of the observation target object candidate from the telescope over status data indicating the status of the sky of the optical telescope inputted from the outside, including the height of the observation target object candidate An unobservable range determining unit that determines an unobservable range, an observable range determining unit that determines an observable range that is observable by the optical telescope from the maximum observable range data and the unobservable range, and the observation target observation availability determination for generating the observable range and the observation capability determination image is an image obtained by superimposing said predicted trajectory of the height of the object candidate It is obtained by a image generation unit.

  According to the present invention, it is possible to support an operator to create an observation plan for artificial satellites, debris, and the like using an optical telescope in consideration of the actual situation over the place where the optical telescope is installed.

It is a block diagram of the system which assists an operator creating the observation plan of the optical telescope which concerns on Embodiment 1 of this invention. 3 is a block diagram illustrating a functional configuration of an observation plan creation support device for an optical telescope according to Embodiment 1. FIG. It is a figure explaining the relationship between the image acquired with the all-sky camera which the observation plan preparation assistance system which concerns on Embodiment 1 has, and an observable range. It is a figure explaining the relationship between the height of an observation target object candidate and the maximum observable range in the observation plan creation support system according to Embodiment 1. It is an example of display on the map of the predicted orbit and the observable range of the observation target object candidate in the observation plan creation support system according to the first embodiment. It is a block diagram showing the functional structure of the observation plan preparation assistance apparatus of the optical telescope which concerns on Embodiment 2 of this invention. It is a block diagram showing the functional structure of the observation plan preparation assistance apparatus of the optical telescope which concerns on Embodiment 3 of this invention. It is an example of display on the map of the orbit of the observation target object candidate and the observable range in the observation plan creation support system according to Embodiment 3.

Embodiment 1
FIG. 1 is a configuration diagram of a system that assists an operator in creating an observation plan for an optical telescope according to Embodiment 1 of the present invention. The observation plan creation support system 100 includes an all-sky camera 2, an observation plan creation support device 3, and a display device 4, each installed at a place where one or more optical telescopes 1 are installed. The observation plan creation support device 3 supports the creation of an observation plan for the night before starting the nightly observation. In this specification, from the time determined before the sunset time to the same time of the next day on the day including the sunset time of the night to be observed is referred to as “night”.

  The optical telescope 1 directs the direction of an observation object such as an artificial satellite or debris based on the observation plan 5 of the night, tracks the movement of the observation object, and a CCD (Charge-Coupled Device) image sensor or the like. An image is acquired by the image sensor. The all-sky camera 2 captures a telescope sky image 6 that is an image above the place where the optical telescope 1 is installed. The all-sky camera 2 has a wide-field optical system such as a fish-eye lens so that the sky above the place where the optical telescope 1 is installed has a sensitivity in one or both of the visible light region and the infrared region. The telescope sky image 6 is telescope sky situation data indicating the sky situation of the optical telescope 1. The all-sky camera 2 is a telescope sky status data acquisition device that acquires telescope sky status data. Other types of telescope sky situation data may be used.

  The observation plan creation support device 3 receives the telescope aerial image 6 from the all-sky camera 2 and the observation object candidate 7 determined by a higher-level device. The observation object candidate 7 is determined by a higher-level device according to the observation progress of the previous week and this week based on the annual plan, monthly plan and weekly plan of observation. A telescope aerial image 6 is captured by the all-sky camera 2 at a predetermined time of the night, for example, 3 hours before sunset, and an observation availability determination image 8 created based on the captured telescope aerial image 6 is seen. The operator prepares the observation plan 5 for the night. The telescope aerial image 6 can be acquired at an arbitrary time according to an instruction from the operator.

  The observation plan creation support device 3 determines an observable range 9 that is an observable range from the telescope aerial image 6 and superimposes the observable range 9 and the predicted orbit 10 of the observation object candidate 7. An observability determination image 8 (an example is shown in FIG. 5), which is an image, is created. The observation availability determination image 8 is displayed on the display device 4 at the request of the operator. An operator who makes a decision by looking at the observation availability determination image 8 displayed on the display device 4 determines the observation plan 5. The determined observation plan 5 is distributed to the optical telescope 1, and the optical telescope 1 observes the observation object according to the observation plan 5.

  FIG. 2 is a block diagram illustrating a functional configuration of the observation plan creation support apparatus for the optical telescope according to the first embodiment. The observation plan creation support apparatus 3 includes a telescope data storage unit 11, a predicted orbit storage unit 12, an unobservable range determination unit 13, an observable range determination unit 14, an observability determination image generation unit 15, an earth surface data storage unit 16, an observation An observation plan candidate determination unit 18 that determines an observation plan candidate 17 including the object candidate 7 and the optical telescope 1 that observes the object candidate 7, and data that drives the optical telescope 1 when executing the observation plan 5 determined by the operator It has a telescope drive data generator 20 that generates certain telescope drive data 19.

  The telescope data storage unit 11 stores telescope data 21 that is data related to the optical telescope 1. The predicted orbit storage unit 12 stores data of observation object candidates 7 such as artificial satellites and debris. The unobservable range determination unit 13 determines an unobservable range 22 that is a range in which the telescope sky image 6 or the like is input and cannot be observed. The observable range determination unit 14 receives the unobservable range 22 and determines the observable range 9 that is the observable range of the optical telescope 1 with reference to the telescope data 21. The observation availability determination image generation unit 15 generates an observation availability determination image 8. The earth surface data storage unit 16 stores the earth surface data in a predetermined range in which the installation position of the optical telescope 1 is entered.

  The telescope data storage unit 11 stores telescope data 21 including latitude, longitude and altitude of the place where the optical telescope 1 is installed, data such as surrounding terrain and structures, driving range of the optical telescope 1 and performance of the driving mechanism, and the like. Is done. Depending on the driving range of the optical telescope 1 and the surrounding topography and structures, the range that cannot be fixedly observed by the telescope is determined. The maximum observable range 23 is a range obtained by removing a range in which the optical telescope 1 is centered and facing the zenith direction from the hemisphere that cannot be fixedly observed. The telescope data 21 includes maximum observable range data 24 that is data for determining the maximum observable range 23.

  The optical telescope 1 can face any direction of 360 degrees in all directions, and the elevation angle can point in any direction from 0 degrees that is the horizontal direction to 90 degrees that is the direction toward the zenith in any direction. In each direction, celestial bodies cannot be observed from the horizontal plane up to the maximum elevation angle obstructed by topography and structures existing in that direction. That is, there is a minimum observable elevation angle that is the minimum observable elevation angle for each azimuth. An elevation angle range smaller than the minimum observable elevation angle is a range in which fixed observation is not possible. Further, the range of elevation angles larger than the minimum observable elevation angle determined for each azimuth is the maximum observable range 23. The data of the minimum observable elevation angle determined for each azimuth becomes the maximum observable range data 24. The maximum observable range data 24 may be in any format as long as it represents an area that cannot be fixedly observed.

  The predicted orbit storage unit 12 stores data for each observation target candidate 7 such as an artificial satellite or debris. The stored data includes the predicted trajectory of the night including the altitude, the priority of observation determined by the host device, the brightness at the time of observation, the date and time that can be observed next to the night, and the like. The predicted trajectory storage unit 12 is also an observation object candidate data storage unit that stores data related to observation object candidates.

  The all-sky camera 2 has an angle of view of 180 degrees, and has an equidistant projection type fisheye lens in which the angle is proportional to the distance from the center of the screen. A fish-eye lens other than the equidistant projection method may be used. The all-sky camera 2 is installed so that the optical axis of the fisheye lens faces in the vertical direction. The telescope aerial image 6 taken by the omnidirectional camera 2 has a circular shape with the zenith corresponding to the center. An image in a 360-degree direction on the horizontal plane is the outer periphery of the telescope aerial image 6. In the case of the equidistant projection method, the distance from the center in the circle is proportional to the angle from the zenith direction of the optical telescope. The unobservable range 22 and the observable range 9 are represented by one or a plurality of ranges represented by the azimuth and elevation ranges in accordance with the image captured by the omnidirectional camera 2. The actual observable range 9 is a space expressed by combining the closed curves representing the azimuth angle and the elevation angle range and the cone connecting the installation location of the optical telescope 1.

  The unobservable range determining unit 13 includes a cloud region determining unit 25, a moon vicinity determining unit 26, and a variable unobservable range determining unit 27. The cloud area determination unit 25 performs image processing on the telescope sky image 6 to determine a cloud area 28 that is an area that cannot be observed due to the presence of clouds and the like. The lunar vicinity determination unit 26 determines a lunar vicinity range 29 that is a predetermined range near the moon that cannot be observed due to the moonlight. The variable observable range determination unit 27 determines a observable range that varies depending on the situation due to the influence of city lights and the like.

  The cloud region determination unit 25 performs image processing on the telescope sky image 6 that is an image above the optical telescope 1 captured by the omnidirectional camera 2 to determine a cloud region 28 that cannot be observed due to the presence of clouds and the like. To do. As the cloud region 28, not only a cloud but also a region that cannot be observed due to a phenomenon such as fog, haze, hail, smog, volcanic plume is extracted from the telescope aerial image 6. In the cloud area determination unit 25, when the omnidirectional camera 2 captures the visible light, the cloud area 28 is determined using the fact that the clouds are brighter than the background space due to the reflection of light on the ground. When photographing with infrared rays, the fact that the temperature of the clouds is higher than the temperature of the outer space is used. In addition, the presence of the cloud region 28 can be predicted indirectly because the background star is shielded and cannot be observed.

  If the telescope aerial image 6 is captured at a plurality of times, the cloud region 28 is extracted for each telescope aerial image 6. The cloud moving speed is estimated from the difference between the extracted cloud areas 28, the estimated moving speed is used to estimate the cloud area 28 at different times, and the estimated cloud area 28 is used to observe the time. The availability determination image 8 may be created.

  Although depending on the brightness of the observation object candidate 7, if the dark observation object candidate 7 exists near the moon, the observation object candidate 7 cannot be observed due to the influence of the brightness of the moon. The lunar vicinity determination unit 26 refers to lunar orbit data including the brightness of the observation object candidate 7 and the predicted orbit of the moon, and determines the lunar vicinity range 29 that cannot be observed due to the influence of the moon.

  Also, for example, if the city lights are bright until midnight, the elevation angle range determined from the boundary of the maximum observable range 23 until midnight in the azimuth range determined in a certain direction of the city. Must be unobservable. The unobservable range 22 due to a streetlight or the like is stored as variable unobservable range data 30 that is data of a time zone and a range where observation is impossible. The variable observable range determination unit 27 refers to the variable observable range data 30 and determines the variable observable range 31. The sum of the cloud region 28, the lunar vicinity range 29, and the variable observable range 31 is the unobservable range 22.

  FIG. 3 is a diagram for explaining the relationship between an image acquired by an all-sky camera and an observable range included in the observation plan creation support system according to the first embodiment. FIG. 3A shows that the minimum observable elevation angle in a certain direction (here, east) is θ degrees. There are trees on the east side, and the elevation angle range lower than the trees is the range that cannot be fixedly observed. FIG. 3B shows an example of the telescope aerial image 6 that is one circular area. The boundary in the east direction of the maximum observable range 23, which is a range obtained by excluding the range in which the optical telescope 1 can not be fixedly fixed, is from the outer periphery of the circle, where r is the radius of the circle of the telescope aerial image 6. It becomes an inner point by a distance of r * (θ / 90). The observable minimum elevation angle often changes depending on the azimuth, but a line connecting the observable minimum elevation angle for each azimuth is a single closed curve. That is, the boundary of the maximum observable range 23 is represented as one closed curve in the telescope aerial image 6 as shown in FIG.

  In FIG. 3B, a cloud region 28 is also shown. In FIG. 3B, the cloud region 28 is represented by a quadrangle, but actually, the cloud region 28 is set in units of regions obtained by dividing the azimuth angle and the elevation angle by a predetermined step size. In the south direction (lower side in the figure), there is a variable non-observable range 31 created from the variable non-observable range data 30 due to the influence of city lights. There is a lunar neighborhood 29 in the southeast direction. The sum of the cloud region 28, the lunar vicinity range 29, and the variable observable range 31 is the unobservable range 22. The observable range 9 is obtained by removing the range that overlaps the unobservable range 22 from the maximum observable range 23.

  The observable range determination unit 14 determines a range obtained by removing the unobservable range 22 from the maximum observable range 23 as the observable range 9 of the optical telescope 1.

  The observability determination image generation unit 15 generates an observability determination image 8 in which the observable range 9 of the optical telescope 1 and the predicted trajectory 10 of the observation object candidate 7 are superimposed. The observation feasibility determination image 8 is created by referring to the earth surface data storage unit 16 and looking down the observable range 9 and the predicted orbit 10 from outside the earth. The method of looking down from the outside of the earth is easier to understand the relationship between the observable range 9 and the predicted orbit 10 than the method of looking up the celestial sphere from the position of the optical telescope 1. For each optical telescope 1, an observability determination image 8 that displays the observable range 9 and the predicted orbit 10 may be created by a method of looking up at the celestial sphere or another method. When the observation possibility determination image 8 is created for each optical telescope 1, the predicted trajectories 10 of the plurality of observation object candidates 7 may be displayed in a superimposed manner.

  The earth surface data storage unit 16 stores data of the earth surface within a predetermined range where all the optical telescopes 1 are installed. When the optical telescope 1 is installed in Japan, for example, earth surface data in a range from 100 degrees to 180 degrees east longitude and from 0 degrees to 90 degrees north latitude is stored. The earth surface data may be displayed as a map or a satellite image.

  In the observability determination image 8, each point on the predicted trajectory 10 of the observation object candidate 7 is drawn at the position of the intersection of the line segment connecting the point and the center of the earth and the earth surface. The topography of the earth surface is also displayed. By doing so, the predicted orbit 10 is drawn on the surface of the earth, and it looks as if the predicted orbit 10 was looked down from outside the earth. The predicted trajectory 10 of the observation object candidate 7 is represented as a line segment, assuming not an instantaneous observation but an observation with a certain time width. Note that the predicted trajectory 10 of the observation object candidate 7 at an altitude close to a geosynchronous trajectory is represented as a point or a short line segment. Conversely, in the case of the observation object candidate 7 at a low altitude, the line segment of the predicted trajectory 10 becomes long.

  The observable range 9 of the optical telescope 1 also includes one or more virtual closed curves in a circle centered at a point in the zenith direction at the installation location of the optical telescope 1 existing at the same altitude as the observation object candidate 7. Think. A closed curve is drawn at a position where a line segment connecting each point on the closed curve and the center of the earth intersects the surface of the earth. This is because the boundary of the observable range 9 determined by the ridgeline of the surrounding mountain, the cloud region 28, etc. is projected onto a spherical screen existing at the same altitude as the observation object candidate 7, and the spherical screen is projected together with the projected image. This corresponds to a case where the image is reduced to coincide with the surface of the earth and the image reflected on the screen is viewed from outside the earth. If there are a cloud region 28 and a lunar vicinity range 29 separated from the boundary of the maximum observable range 23, there will be a plurality of closed curves representing the observable range 9.

  FIG. 4 is a diagram for explaining the relationship between the observation target candidate altitude and the observable range in the observation plan creation support system according to the first embodiment. As shown in FIG. 4, the region representing the observable range 9 on the map increases as the altitude of the observation object candidate 7 increases.

  Since the size of the observable range 9 varies depending on the altitude, the observability determination image 8 is created for each observation object candidate 7. In the case of the observation object candidate 7 having an altitude change, the observable range 9 is created by synthesizing observable ranges 9 having different altitudes so that the portion where the observable range 9 and the predicted orbit 10 intersect is as accurate as possible. . Note that the predicted trajectory 10 and the observable range 9 of the plurality of observation object candidates 7 may be displayed at the same time so that they can be distinguished by changing colors.

  The observation possibility determination image 8 may be one for each observation object candidate 7 that night, or the observation possibility determination images 8 at a plurality of times may be created and displayed as animations.

  The observation plan candidate determination unit 18 determines whether or not the predicted orbit 10 of the observation object candidate 7 is included in the observable range 9. When the observable range 9 including the predicted orbit 10 of the observation object candidate 7 exists, the observation plan including the optical telescope 1 having the observable range 9 and the observation object candidate 7 corresponding to the predicted orbit 10 Candidate 17 is determined. The data of the observation plan candidate 17 also includes data indicating whether or not there is an observation plan candidate 17 that has a relationship in which both cannot be executed because the observable time zones overlap.

  The telescope drive data generation unit 20 generates telescope drive data 19 for driving the optical telescope 1 when the observation plan 5 is executed. The generated telescope drive data 19 is transmitted to a device that drives the optical telescope 1 as part of the observation plan 5, and the optical telescope 1 is driven according to the telescope drive data 19, and the observation target determined in the observation plan 5 Observe things.

  The operation will be described. The all-sky camera 2 captures the telescopic aerial image 6 at a predetermined time of the night. The telescopic aerial image 6 may be taken not only once but multiple times. The observation plan creation support device 3 is automatically activated at a predetermined time of the night, and whether or not the observation object candidate 7 input at or before that time can be observed using the telescope aerial image 6 A judgment image 8 and an observation plan candidate 17 are created. Note that the observation plan creation support apparatus 3 may be started manually by the operator.

  The unobservable range determination unit 13 determines the unobservable range 22 from the telescope aerial image 6 or the like. The observable range determination unit 14 determines the maximum observable range 23 with reference to the maximum observable range data 24 and determines the observable range 9 as a range obtained by removing the unobservable range 22 from the maximum observable range 23. The observability determination image generation unit 15 generates an observability determination image 8 for each observation object candidate 7 using the observable range 9 and the predicted trajectory 10 of the observation object candidate 7. The observation plan candidate determination unit 18 determines whether or not the predicted orbit 10 of the observation object candidate 7 is included in the observable range 9 and determines the observation plan candidate 17.

  FIG. 5 is a display example on the map of the predicted trajectory and the observable range of the observation target object candidate in the observation plan creation support system according to the first embodiment. FIG. 5 shows a case where the observation object candidate 7 is in a low orbit. In FIG. 5, two observable ranges 9 of the optical telescope 1 are drawn on the assumption that two optical telescopes 1 are installed at distant locations. Each observable range 9 is a range obtained by removing the observable range 22 represented by a square from the maximum observable range 23 represented by a circle. This means that when the line segment indicating the predicted trajectory 10 of the observation object candidate 7 crosses the boundary of the two observable ranges 9 or exists inside the observable range 9, the observation can be performed with the optical telescope 1 having the observable range 9. To do.

  In the case of the observation target candidate 7 in the high orbit, the radius of the circle indicating the observable range 9 is large, and the predicted orbit 10 is set in a range where the observable ranges 9 of the plurality of optical telescopes 1 installed at distant locations overlap. There may be a line segment to represent. In this case, it is possible to simultaneously observe the observation object candidate 7 with a plurality of optical telescopes 1. In the observability determination image 8, when simultaneous observation is possible, it is displayed as a case where the predicted trajectory 10 enters a range where a plurality of observable ranges 9 overlap. The operator can easily determine whether or not simultaneous observation is possible by creating the observation availability determination image 8 and presenting it to the operator. Note that by observing simultaneously with a plurality of optical telescopes 1, the altitude, shape, orbit, etc. of the observation object candidate 7 can be observed more accurately than when observing with a single optical telescope 1.

  The operator selects the observation object candidate 7 and displays the observation availability determination image 8 on the display device 4. The operator confirms the length of the line segment of the predicted orbit 10 of the observation object candidate 7 included in the observable range 9 and determines whether or not the observation plan candidate 17 for observing the observation object candidate 7 can be implemented. To do. The operator refers to the observation possibility determination image 8 and modifies the observation plan candidate 17 as necessary to determine the observation plan 5 for the night.

  Since the predicted trajectory 10 and the observable range 9 are simultaneously displayed on the map, the operator can easily determine whether the observation is possible. Since the observable range 9 is set in consideration of the variable non-observable range 22 such as a cloud, it can be determined whether or not the observation is possible in consideration of the sky condition of the optical telescope 1 on that day.

  When the observation plan 5 is determined by the operator, the telescope drive data generation unit 20 generates telescope drive data 19 for implementing the observation plan 5. The generated telescope drive data 19 is input to a device that drives the optical telescope 1 via a network. The optical telescope 1 is driven according to the telescope drive data 19 and observes the observation object candidate 7. The telescope drive data 19 may be created when the observation plan candidate 17 is created.

  Even after deciding the observation plan 5 for the night, the telescope sky image 6 can be taken and the observation availability determination image 8 can be created from the telescope sky image 6 according to the operator's instruction. The unobservable range 22 such as the cloud region 28 varies with time, and by redrawing the observability determination image 8 in accordance with the observable range 9 that changes in accordance with it, it is determined whether observation is possible from moment to moment. Judgment can be made.

  The observation plan support apparatus may not have the observation plan candidate determination unit. All observation plans may be created by the operator. The telescope drive data generation unit may not be provided. In that case, another device to which the observation plan is input generates telescope drive data. The telescope drive data may be generated by a device on the optical telescope side to which an observation plan is given.

  The unobservable range determining unit 13 may have any configuration as long as the unobservable range 22 of the optical telescope 1 can be determined from the telescope sky status data indicating the sky status of the optical telescope 1. The range near the moon that cannot be observed due to the influence of the moon need not be determined as the unobservable range. It is not necessary to obtain the variable observable range based on the time zone and the data of the observable range.

The observation plan support apparatus is realized by mounting dedicated software for realizing each functional unit on one or a plurality of general-purpose computers. The computer has a central processing unit (CPU), a memory, a nonvolatile storage device, and the like. The storage unit that stores various types of data may store the data dispersed in a plurality of storage devices.
The above also applies to other embodiments.

Embodiment 2. FIG.
In the second embodiment, an observation apparatus that can measure the actual cloud position with high resolution in real time, for example, observation data of a lidar (LIDAR, Light Detection and Ranging) is used to set an unobservable range due to weather conditions such as clouds. This is the case. FIG. 6 is a block diagram showing a functional configuration of an observation plan creation support apparatus for an optical telescope according to Embodiment 2 of the present invention. Only the differences from the first embodiment will be described.

  The rider 32 is a radar that radiates laser light into the air, receives reflected light obtained by reflecting the emitted light by aerosol in the air, and measures clouds in the air. The rider 32 measures a cloud in a predetermined spatial range including the sky above the optical telescope 1 with a determined resolution, and generates telescope on-air image data 33 that is three-dimensional numerical data. The telescope air image data 33 is telescope sky condition data indicating the condition of the optical telescope 1 above. The rider 32 is a telescope sky condition data acquisition device that acquires telescope sky condition data.

  The optical telescope observation plan creation support apparatus 3 </ b> A according to the second embodiment includes a cloud region generation unit 34. The cloud region generation unit 34 numerically converts the telescope on-air image data 33 and generates an unobservable range 22 in the image when the fisheye lens is used to capture images from the position of the optical telescope 1. After generating the unobservable range 22, the operation is the same as in the first embodiment.

  Even if the rider 32 is not necessarily installed at the same location as the optical telescope 1, it can numerically calculate the cloud distribution in the sky facing the installation location of the optical telescope 1. It is easier to predict future cloud distribution by assuming cloud flow based on the cloud position data of the night or in the past.

  Instead of a rider, a radar using radio waves or sound waves may be used. If sufficiently high time and space resolution can be achieved, observation data from artificial satellites may be used in the future. Any kind of data may be used as long as it can measure the situation affecting the availability of observation over the optical telescope.

Embodiment 3 FIG.
The third embodiment is a case where an observable range can be generated with respect to an installation position of an optical telescope virtually input so that it can be used when planning the installation of a new optical telescope 1. .

  FIG. 7 is a block diagram showing a functional configuration of an observation plan creation support apparatus for an optical telescope according to Embodiment 3 of the present invention. Only differences from FIG. 2 in the first embodiment will be described. The optical telescope observation plan creation support apparatus 3B according to the second embodiment includes a virtual telescope data storage unit 36 that stores virtual telescope data 35 of a virtual optical telescope input by an operator. As the virtual telescope data 35, at least the installation location is stored. The virtual maximum observable range 37, which is the maximum observable range of the virtual optical telescope, is generated from the minimum observable elevation angle input by the operator in all directions or uniformly for each direction. If the operator does not input, the default value in all directions is used as the minimum observable elevation angle. By specifying the installation location correctly, the virtual maximum observable range 37 may be determined from the earth surface data around the installation location.

  The observability determination image generation unit 15A also superimposes and displays the virtual maximum observable range 37 generated from the virtual telescope data 35. The predicted trajectory 10 acquires the predicted trajectory of the observation target designated by the operator from the predicted trajectory storage unit 13. FIG. 8 is a display example on the map of the trajectory of the observation object candidate and the observable range in the observation plan creation support system according to the third embodiment. The virtual maximum observable range 37 of the optical telescope input virtually is indicated by a dotted line in FIG. 8, and the installation location of the virtual optical telescope is also indicated by a dotted line. The predicted orbit 10 and the observable range 9 of the actual optical telescope 1 may be displayed using data obtained in the past observation.

  Since it is possible to determine whether or not the observation target object can be observed with the virtually input optical telescope, the observable range after the newly installed optical telescope can be evaluated in advance. Since the installation location can be freely set and examined, the possibility of installing the optical telescope in a better location can be increased.

  The virtual telescope data 35 may be stored in the telescope data storage unit 11 after being distinguished from the telescope data 21 of the actual optical telescope 1. In that case, the telescope data storage unit 11 is also a virtual telescope data storage unit. The observable range determination unit determines the observable range by distinguishing whether the telescope data 21 is real or virtual. The observable range for the virtual telescope data 35 is the virtual maximum observable range.

  The present invention can be freely combined with each other, or can be modified or omitted within the spirit of the invention.

100, 100A, 100B Observation plan creation support system 1 Optical telescope 2 All-sky camera 3, 3A, 3B Observation plan creation support device 4 Display device 5 Observation plan 6 Telescope sky image (telescope sky status data)
7 Observation Object Candidate 8 Observability Determination Image 9 Observable Range 10 Predicted Trajectory 11 Telescope Data Storage Unit 12 Prediction Orbit Storage Unit (Observation Object Candidate Data Storage Unit)
13 Observable range determination unit 14 Observable range determination unit 15, 15 A Observation availability determination image generation unit 16 Earth surface data storage unit 17 Observation plan candidate 18 Observation plan candidate determination unit 19 Telescope drive data 20 Telescope drive data generation unit 21 Telescope data 22 Unobservable range 23 Maximum observable range 24 Maximum observable range data 25 Cloud region determination unit 26 Moon vicinity determination unit 27 Variable observable range determination unit 28 Cloud region 29 Moon vicinity range 30 Variable observable range data 31 Variable observable range 32 Rider 33 Telescope Air Elephant Data (Telescope Air Condition Data)
34 Cloud region generation unit 35 Virtual telescope data 36 Virtual telescope data storage unit 37 Virtual maximum observable range

Claims (10)

A telescope data storage unit for storing telescope data including a maximum observable range data, which is data for determining an installation location of the optical telescope, and a maximum observable range of the optical telescope;
And it predicted orbit storage unit for storing a predicted trajectory that includes the height of the observation target object candidate for each of the observation target object candidates,
An unobservable range determination unit that determines an unobservable range of the optical telescope from telescope sky status data indicating the sky status of the optical telescope input from the outside;
An observable range determination unit that determines an observable range that is observable by the optical telescope from the maximum observable range data and the non-observable range;
Support for creating an observation plan for an optical telescope including an observation availability determination image generation unit that generates an observation availability determination image that is an image obtained by superimposing the observation range and the predicted trajectory at the height of the observation target candidate apparatus. An earth surface data storage unit for storing data of a predetermined range of the earth surface including the installation location of the optical telescope;
In the observability determination image, the observable range and the predicted trajectory are set at the intersection of the line segment connecting the position of the observation target candidate at the height of the predicted trajectory and the center of the earth and the earth surface. The optical telescope observation plan creation support apparatus according to claim 1, wherein the optical telescope observation plan creation support apparatus displays the observation plan.   The observation plan candidate determining unit for determining an observation plan candidate including the optical telescope having the observable range in which the predicted trajectory is included and the observation object candidate corresponding to the predicted trajectory. The observation plan creation support apparatus of the optical telescope according to claim 2. An observation object candidate data storage unit for storing data relating to the observation object candidate;
4. The observation plan creation support apparatus for an optical telescope according to claim 3, wherein the observation plan candidate determination unit determines the observation plan candidate with reference to the observation target candidate data storage unit.   The optical telescope observation plan creation support apparatus according to any one of claims 1 to 4, wherein the telescope sky situation data is an image obtained by photographing the sky of the optical telescope.   5. The optical telescope observation plan creation support apparatus according to claim 1, wherein the telescope sky condition data is data obtained by measuring the sky above the optical telescope with a radar. 6. A virtual telescope data storage unit for storing virtual telescope data including the installation location of the virtual optical telescope input from the outside;
The observability determination image generation unit generates the observability determination image by superimposing a virtual maximum observable range generated from the virtual telescope data stored in a virtual telescope data storage unit. The observation plan creation support device for an optical telescope according to any one of claims 1 to 6. An observation plan creation support device for an optical telescope according to any one of claims 1 to 7,
A telescope sky condition data acquisition device for acquiring the telescope sky condition data ;
Observation planning support system of the optical telescope and a display device for displaying the previous SL observation possibility determination image. An observation plan creation support device for an optical telescope according to claim 5,
A camera that takes an image of the sky above the optical telescope and inputs it to the observation plan creation support device as the sky status data of the telescope ;
Observation planning support system of the optical telescope and a display device for displaying the previous SL observation possibility determination image. An observation plan creation support device for an optical telescope according to claim 6,
A radar that measures the sky above the optical telescope and inputs the measured data to the observation plan creation support device as the telescope sky status data ;
Observation planning support system of the optical telescope and a display device for displaying the previous SL observation possibility determination image.

Images