Wolfram Function Repository
Instant-use add-on functions for the Wolfram Language
Function Repository Resource:
Retrieve images of the Sun from many NASA/ESA scientific instruments
ResourceFunction["SolarImage"][] returns the current HMI intensitygram of the Sun. | |
ResourceFunction["SolarImage"][date] returns the HMI intensitygram for the specified date. | |
ResourceFunction["SolarImage"][instcode] returns a current solar image from the instrument specified by instcode. | |
ResourceFunction["SolarImage"][date,instcode] returns a solar image for the specified instcode and date. |
| "BlendColors" | Automatic | colors to blend together to colorize the resulting image |
| "Colorize" | Automatic | whether to colorize black and white images |
| ImageSize | Medium | image size of the resulting image |
| 0 | SOHO EIT 171 (1996/01/05–2013/08/07) |
| 1 | SOHO EIT 195 (1996/01/05–2013/08/07) |
| 2 | SOHO EIT 284 (1996/01/05–2013/08/07) |
| 3 | SOHO EIT 304 (1996/01/05–2013/08/07) |
| 4 | SOHO LASCO C2 (1996/04/01–present) |
| 5 | SOHO LASCO C3 (1996/04/14–present) |
| 6 | SOHO MDI Mag (1996/05/19–2011/01/11) |
| 7 | SOHO MDI Int (1996/05/19–2011/01/11) |
| 8 | SDO AIA 94 (2010/06/02–present) |
| 9 | SDO AIA 131 (2010/06/02–present) |
| 10 | SDO AIA 171 (2010/06/02–present) |
| 11 | SDO AIA 193 (2010/06/02–present) |
| 12 | SDO AIA 211 (2010/06/02–present) |
| 13 | SDO AIA 304 (2010/06/02–present) |
| 14 | SDO AIA 335 (2010/06/02–present) |
| 15 | SDO AIA 1600 (2010/06/02–present) |
| 16 | SDO AIA 1700 (2010/06/02–present) |
| 17 | SDO AIA 4500 (2010/06/02–present) |
| 18 | SDO HMI Int (2010/12/06–present) |
| 19 | SDO HMI Mag (2010/12/06–present) |
| 20 | STEREO EUVI-A 171 |
| 21 | STEREO EUVI-A 195 |
| 22 | STEREO EUVI-A 284 |
| 23 | STEREO EUVI-A 304 |
| 24 | STEREO EUVI-B 171 |
| 25 | STEREO EUVI-B 195 |
| 26 | STEREO EUVI-B 284 |
| 27 | STEREO EUVI-B 304 |
| 28 | STEREO COR1-A |
| 29 | STEREO COR2-A |
| 30 | STEREO COR1-B |
| 31 | STEREO COR2-B |
| 32 | SWAP 174 |
| 33 | SXT AlMgMn |
| 34 | SXT thin-Al |
| 35 | SXT white-light |
| 39 | Hinode XRT Al_med/Al_thick |
| 40 | Hinode XRT Al_med/Be_thick |
| 42 | Hinode XRT Al_med/Open |
| 43 | Hinode XRT Al_med/Ti_poly |
| 44 | Hinode XRT Al_poly/Al_mesh |
| 45 | Hinode XRT Al_poly/Al_thick |
| 46 | Hinode XRT Al_poly/Be_thick |
| 48 | Hinode XRT Al_poly/Open |
| 49 | Hinode XRT Al_poly/Ti_poly |
| 54 | Hinode XRT Be_med/Open |
| 62 | Hinode XRT C_poly/Al_mesh |
| 63 | Hinode XRT C_poly/Al_thick |
| 66 | Hinode XRT C_poly/Open |
| 67 | Hinode XRT C_poly/Ti_poly |
| 69 | Hinode XRT Open/Al_mesh |
| 70 | Hinode XRT Open/Al_thick |
| 71 | Hinode XRT Open/Be_thick |
| 74 | Hinode XRT Open/Ti_poly |
| 75 | TRACE 171 |
| 76 | TRACE 195 |
| 77 | TRACE 284 |
| 78 | TRACE 1216 |
| 79 | TRACE 1550 |
| 80 | TRACE 1600 |
| 81 | TRACE 1700 |
| 82 | TRACE white-light |
| 83 | COSMO KCor |
| 2000 | SUVI 94 |
| 2001 | SUVI 131 |
| 2002 | SUVI 171 |
| 2003 | SUVI 195 |
| 2004 | SUVI 284 |
| 2005 | SUVI 304 |
| 10001 | Hinode XRT Any/Any |
| 10002 | Hinode XRT Any/Al_mesh |
| 10003 | Hinode XRT Any/Al_thick |
| 10004 | Hinode XRT Any/Be_thick |
| 10005 | Hinode XRT Any/Gband |
| 10006 | Hinode XRT Any/Open |
| 10007 | Hinode XRT Any/Ti_poly |
| 10008 | Hinode XRT Al_med/Any |
| 10009 | Hinode XRT Al_poly/Any |
| 10010 | Hinode XRT Be_med/Any |
| 10011 | Hinode XRT Be_thin/Any XRT Be_thin/Open |
| 10012 | Hinode XRT C_poly/Any |
| 10013 | Hinode XRT Open/Any |
Get a current image of the Sun from the Helioseismic and Magnetic Imager (HMI) on the Solar Dynamics Observatory (SDO):
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Get a current image of the Sun from the Atmospheric Imaging Assembly (AIA) at 94 angstroms on SDO:
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Get an image of the sun from the SunSDO HMI Int on a specific date:
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Get older images of the Sun from the SOHO mission:
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Choose images from many different instruments:
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For some instrument codes, "Colorize" can be used to colorize black and white images automatically:
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"BlendColors" can be used to specify or override the colors used by "Colorize":
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The AIA 94 Angström instrument can show images of solar flares:
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SpaceWeatherData can also view solar flares by plotting the X-ray emission and observing sudden spikes:
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This work is licensed under a Creative Commons Attribution 4.0 International License