Morphological catalog of prominences observed by the MFS&HSFA at Ondrejov for 1998 - 2017 year (ver. 0.4)


Time is in UT. Data from NOAA SEC and other sources are given.

Made by Yu. A. Kupryakov, P. Kotrč , L.K. Kashapova in 2013-2018.

Annotation

Programs for the construction of spectral line profiles and determination of radial velocities : xlook.pro, vel_eva.pro

Modeling of plasma motion    download program  

1998-2008 2011 2012 2013-1015 2015-2016 2017

MFS


1998

Date (YYYYMMDD) Start

MFS

End

MFS

Type Solar Activity Monitoring and Forecasting SOHO Global High-Resolution H-alpha Network Note
19980602 0533 0955 IIa Common Eruptive 08:27 UT 09:19:20 UT / 09:19:24 UT / 09:19:32 UT + + [9]

1999

Date (YYYYMMDD) Start

MFS

End

MFS

Type BASS2000 H Alpha coronographic image SOHO Global High-Resolution H-alpha Network Note
19990713 0925 1101 IVb Skeleton Tornado +   +    
19990717 1046 1104 IIb1 Common Eruptive + + +    

2000

Date (YYYYMMDD) Start

MFS

End

MFS

Type BASS2000 H Alpha coronographic image SOHO SSC Global High-Resolution H-alpha Network Note
20000407 0915 0925 Ia Interactive + +     +  
20000501 0552 0752 Ic Coronal Active +   +   +  
20000801 0452 0812 V Quiescent + + +   +  
20000801 0708 1131 Ia Interactive + + +   +  
20000801 0716 0742 IVa Columnar Tornado + + +   +  
20000802 0530 0912 IIb2 Common Eruptive +   +   + Stages of development of the prominence 08:30 - 09:13 UT

2001

Date Start

MFS

End

MFS

Type BASS2000 H Alpha coronographic image SOHO SSC Global High-Resolution H-alpha Network Note
20010509 0457 1137 IVb Skeleton Tornado +       +  
20010511 0540 0755 IIb1 Common Eruptive +       +  
20010520 0558 1051 IIb1 Common Eruptive + +        
20010525 0529 0957 Ia Interactive + +        
20010626 0635 1255 IVa Columnar Tornado + +        
20010705 0600 0855 Ic Coronal Active +       +  
20010705 0600 0855 IVa Columnar Tornado +       +  
20010715 0552 0623 Ia Interactive +   +   +  
20011001 1039 1111 IIb1 Common Eruptive +       +  
20011002 0856 1036 Ic Coronal Active + + +   +  
20011002 0856 1036 IIId2 Expanding Surge + + +   +  
20011009 0631 1218 IIb1 Common Eruptive + + +   + 074540 UT 075046 UT

2002

Date Start

MFS

End

MFS

Type BASS2000 H Alpha coronographic image SOHO SSC Global High-Resolution H-alpha Network Note
20020104 0904 1004 IIb1 Common Eruptive +   + + + archiv MFS
20020516 0516 0655 IIa Quasi-Eruptive +     + + archiv MFS
20020625 0610 1204 Ic Coronal Active   +   + +  
20020626 0547 0900 IIa Quasi Eruptive - Columnar Tornado + +   + + velosityarchiv MFS
20020630 1148 1152 Ia Interactive + +   + +  
20020701 1155 1321 IIb1 Common Eruptive + +   + + 171A/ 284A
20020701 1155 1321 IIb1 Common Eruptive + +   + + archiv MFS
20020706 0618 1213 Ib Common Active + +   + +  
20020804 0618 1213 Columnar Tornado + +   + +

2003

Date Start

MFS

End

MFS

Type BASS2000 H Alpha coronographic image SOHO SSC Global High-Resolution H-alpha Network Note
20030425 0538 0556 IIb1 Common Eruptive + + +   + 05:43 UT
20030426 0803 0853 IIb1 Common Eruptive +   +   + 08:23 UT / 08:32 UT / 08:42 UT
20030601 1136 1250 IIb1 Common Eruptive     +   + 12:50 UT
20030602 0507 1038 IIIb Looped Coronal Sunspot     +   + 10:39 UT
20030612 0603 1429 IIb1 Common Eruptive   + +   + 10:52 UT [10]
20030616 1214 1217 IIb1 Common Eruptive +   +      
20030711 0716 1329 IIb1 Common Eruptive   + +   +  
20030720 0707 1205 IIIg Coronal Cloud +   +   +  
20030801 0659 1100 IIId2 Expanding Surge + + +   +  
20030801 1020 1040 IIIg Coronal Cloud + + +   +  
20030915 1031 1415 V Quiescent + + +      
20031023 0810 10013 IIIb Looped Coronal Sunspot + + +   + +

MFS

2004

Date Start

HSFA

End

HSFA

Type BASS2000 H Alpha coronographic image SOHO SSC Global High-Resolution H-alpha Network Note
20040402 0618 1202 Ia Interactive     +   + 11:42 UT
20040423 0558 1213 IVa Columnar Tornado +       + [10]
20040428 0659 0924 Ic Coronal Active       + + +

HSFA

2005

Date Start

HSFA

End

HSFA

Type BASS2000 H Alpha coronographic image SOHO SSC Global High-Resolution H-alpha Network Note
20050620 0712 0803 Ia Interactive + +     +  
20050907 1242 1256 IIId2 Expanding Surge +       +  
20050925 1242 1256 Ia Interactive +          

2006

Date Start

HSFA

End

HSFA

Type BASS2000 H Alpha coronographic image SOHO SSC Global High-Resolution H-alpha Network Note
20060917 0636 0924 Ic Coronal Active - - +   +  
20061111 1120 1157 Ic Coronal Active - - -   +  
20061114 1149 1250 Ic Coronal Active + - +   +  
20061125 1110 1150 Ia Interactive - - +   +  

2007

Date Start

HSFA

End

HSFA

Type BASS2000 H Alpha coronographic image SOHO SSC Global High-Resolution H-alpha Network Note
20070425 0821 1400 V Quiescent + - - + + [6]
20070816 0935 0953 Ia Interactive - - - + +  
20070818 0935 0953 Ia Interactive - - - + +  

2008

Date Start

HSFA

End

HSFA

Type BASS2000 H Alpha coronographic image SOHO SSC Global High-Resolution H-alpha Network Note
20080827 0705 1212 Expanding Surge (Class IIId2) + + + + +  
20080827 0652 0752 Coronal Cloud (Class IIIg) + + + + +  

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Note
Publications:
  • [9] Plunkett S. P., Vourlidas A., Simberova S., Karlicky M., Kotrc P., Heinzel P., Kupryakov Yu.A., Guo W.P., Wu S.T.: 2000; Simultaneous SOHO and Ground-Based Observations of a Large Eruptive Prominence and Coronal Mass Ejection; Solar Physics, Vol. 194, p. 371-391.
    more information
  • Yu. A. Kupryakov, P. Kotrč, 2011, Catalogue of prominences observed by the Solar Laboratory Spectrograph (SLS) at Ondrejov from 16th April till 15 November, 2011
    more information
  • Yu. A. Kupryakov, P. Kotrč, 2013, Catalogue of prominences observed by the Solar Laboratory Spectrograph (SLS) at Ondrejov from 18th April till 24 November, 2012
    more information
  • [1] P. Schwartz, P. Heinzel, P. Kotrč, U. Anzer, Y. Kupryakov, E. DeLuca, Mass Loading of Quiescent Prominences, The Fifth Hinode Science Meeting. ASP Conference Series, Vol. 456, Proceedings of a conference held 10-14 October 2011 at Royal Sonesta Hotel, Cambridge, Massachusetts. Edited by Leon Golub, Ineke De Moortel and Toshifumi Shimizu. San Francisco: Astronomical Society of the Pacific, 2012., p.73
  • [2] Schwartz, Pavol; Heinzel, Peter; Kotrc, Pavel; Farnik, Frantisek; Kupryakov, Yurij A.; DeLuca, Edward E.; Golub, Leon, Total mass loading of prominences estimated from their multi-spectral observations,2014; Nature of Prominences and their role in Space Weather Proceedings IAU Symposium No. 300, 2013 B. Schmieder, J.-M. Malherbe & S. T. Wu, eds.
  • [3] P. Schwartz, P. Heinzel, P. Kotrc, F. Farnik, Yu. A. Kupryakov, E. E. DeLuca:2014: Hmotnost pokojnych protuberancii urcena z multispektralnych pozorovani, Proceedings of the 21st National Solar Physics Meeting,1-6, Stara Tura, Slovakia
  • [4] P. Schwartz, P. Heinzel, P. Kotrc, F. Farnik, Yu. A. Kupryakov, E. E. DeLuca and L. Golub:2015: Total mass of six quiescent prominences estimated from their multi-spectral observations, A&A , Volume 574, February 2015, A62, DOI
  • [5]Kotrc P., Kupryakov Y.A., Barta M., Kashapova L., Wenjuan Liu:2015: Analysis of a limb eruptive event, Coimbra Solar Physics Meeting - CSPM2015, Coimbra, Portugal, 5-9 Oct 2015. more information
  • Schwartz P., Heinzel P., Jejcic S., Rybak J., Kotrc P., Farnik F., Kupryakov Yu A., DeLuca E.E., Golub L., Jibben P.R., Anzer U., Tlatov A.G., Guseva S.A. :2015:Is it possible to use the green coronal line instead of X rays to cancel an effect of the coronal emissivity deficit in estimation of the prominence total mass from decrease of the EUV-corona intensities? ,Coimbra Solar Physics Meeting - CSPM2015, Coimbra, Portugal, 5-9 Oct 2015. more information
  • [6] P. Heinzel, B. Schmieder, F. Farnik, P. Schwartz, N. Labrosse, P. Kotrc, U. Anzer, G. Molodij, A. Berlicki, E. E. DeLuca, L. Golub, T. Watanabe and T. Berger: HINODE, TRACE, SOHO, AND GROUND-BASED OBSERVATIONS OF A QUIESCENT PROMINENCE, The Astrophysical Journal, 686:1383Y1396, 2008 October 20
    more information
  • Schwartz, P.; Heinzel, P.; Jejcic, S.; Rybak, J.; Kotrc, P.; Farnik, F.; Kupryakov, Yu. A.; Deluca, E. E.; Golub, L.; Jibben, P. R. :2016:Is it Possible to Use the Green Coronal Line Instead of X rays to Cancel an Effect of the Coronal Emissivity Deficit in Estimation of the Prominence Total Mass from Decrease of the EUV-corona Intensities? ,Coimbra Solar Physics Meeting: Ground-based Solar Observations in the Space Instrumentation Era Proceedings of a Meeting held at the University of Coimbra, Coimbra, Portugal In 5-9 October 2015. Edited by Ivan Dorotovic, Catherine E. Fischer, and Manuela Temmer. ASP Conference Series, Vol. 504. San Francisco: Astronomical Society of the Pacific, 2016, p.89 more information
  • [7] Kashapova L., Kotrc P., Kupryakov Yu, Barta M.;2016; Analysis results of the limb eruptive events as a signature of a flux-rope formation, 5-th RadioSun Workshop and Summer School,23-27 may 2016, Ceske Budejovice, CR more information
  • [8] Heinzel P., Kupryakov Yu, Schwartz P.; 2016:On the visibility of Mg I lines in solar prominences, XIVth Hvar Astrophysical Colloquium "Solar and Solar-Terrestrial Physics: Now and in the Future" , 26-30 september 2016, Hvar, Croatia more information
  • [8] Heinzel P., Kupryakov Yu, Schwartz P.; 2016:Lines of MgI Detected in Solar Prominences, Central European Astrophysical Bulletin, vol.40,2016, 81-87, DOI: 2016CEAB...40...87H more information
  • [9] P. Kotrc, Yu.A. Kupryakov, L. K. Kashapova;2017; On rotation of prominences observed by ground based spectrographs at Ondcejov, 15-th European Solar Physics Meetings (ESPMs), 04-08 September 2017, Budapest, Hungary. more information
  • [10] Yu. A. Kupryakov, P. Kotrc, L. K. Kashapova, 2018; Investigation of the preflare role of prominences of the "tornado" type on the basis of ground observations of the spectrographs of the Ondzheev Observatory, Conference "Magnetism, cycles of activity and outbreaks on the Sun and stars", June 3-7, 2018, Crimea, pos. Scientific, Crimea. more information
    Please feel free to send your comments or questions to kupry@asu.cas.cz / kupry@sai.msu.ru and pkotrc@asu.cas.cz
    © 2018 Yu. Kupryakov, Pavel Kotrč , L.K. Kashapova