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
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2024
2010
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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
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2010
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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
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2010
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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
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2024
2010
2011
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2000
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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 |