White Light Full-Disk Observation
1918 - 1998: Photographic observation with 20cm Zeiss Refractor at Mitaka (specification is here)
1938 - 1998: Sunspot drawing observation with 20cm Zeiss Refractor at Mitaka (specification is here)
1998 - current: 10cm Refractor wiht a CCD camera at Mitaka
*The observations until May 1998 were test observations, and the data are incomplete and for reference only. Therefore, please do not use it for data analysis.
10cm Refractor: Full-Disk Images (jpg file, 1000x1000 pixels)
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2020
2021
2022
2023
2024
2010
2011
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1997
1998
1999
- The image orientation is celestial north at the top and west to the right.
- The files are named “srYYYYMMDD.jpg”, where ‘YYYYMMDD’ is the date of observation.
| 2020 | 2021 | 2022 | 2023 | 2024 | |||||
| 2010 | 2011 | 2012 | 2013 | 2014 | 2015 | 2016 | 2017 | 2018 | 2019 |
| 2000 | 2001 | 2002 | 2003 | 2004 | 2005 | 2006 | 2007 | 2008 | 2009 |
| 1997 | 1998 | 1999 |
10cm Refractor: Computer-Generated Drawings (postscript file)
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2020
2021
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2010
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2000
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- The image orientation is celestial north at the top and west to the right.
- The files are named “spotYYYYMMDD1.ps”, where ‘YYYYMMDD’ is the date of observation.
- Criteria of the sunspot detection and drawing:
- Individual sunspots are detected based on the criterion that the brightness of two or more neighboring pixels on the CCD falls below a threshold value. Threshold values for the sunspot detection are defined as follows:
- •Penumbra: mi - (6.0×sd) …(a),
- •Umbra: mi - (30.0×sd) …(b),
- where, “mi” and “sd” are the mean and standard deviation of brightness derived from a FITS sdYYYYMMDD.fts, respectively. All features satisfying the threshold (a) are detected as individual sunspots and drawn with contour lines. Areas satisfying the threshold (b) are filled in black as umbrae.
| 2020 | 2021 | 2022 | 2023 | 2024 | |||||
| 2010 | 2011 | 2012 | 2013 | 2014 | 2015 | 2016 | 2017 | 2018 | 2019 |
| 2000 | 2001 | 2002 | 2003 | 2004 | 2005 | 2006 | 2007 | 2008 | 2009 |
| 1997 | 1998 | 1999 |
10cm Refractor: Sunspot (Group) Parameters
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2020
2021
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2024
2010
2011
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1997
1998
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- The files are named “spotYYYYMMDD.txt” or “spotgroupYYYYMMDD.txt” (including parameters of sunspot groups), where ‘YYYYMMDD’ is the date of observation.
| 2020 | 2021 | 2022 | 2023 | 2024 | |||||
| 2010 | 2011 | 2012 | 2013 | 2014 | 2015 | 2016 | 2017 | 2018 | 2019 |
| 2000 | 2001 | 2002 | 2003 | 2004 | 2005 | 2006 | 2007 | 2008 | 2009 |
| 1997 | 1998 | 1999 |
10cm Refractor:Sunspot Area Data, 1998--
10cm Refractor: Full-Disk Images (FITS-format data)
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2020
2021
2022
2023
2024
2010
2011
2012
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2014
2015
2016
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2018
2019
2000
2001
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1997
1998
1999
- The files are named “srYYYYMMDD.fts” or “sdYYYYMMDD.fts” (limb-darkening corrected), where ‘YYYYMMDD’ is the date of observation.
| 2020 | 2021 | 2022 | 2023 | 2024 | |||||
| 2010 | 2011 | 2012 | 2013 | 2014 | 2015 | 2016 | 2017 | 2018 | 2019 |
| 2000 | 2001 | 2002 | 2003 | 2004 | 2005 | 2006 | 2007 | 2008 | 2009 |
| 1997 | 1998 | 1999 |