Published October 1998 | Version public
Journal Article

Properties and Motions of Ellerman Bombs

  • 1. ROR icon California Institute of Technology

Abstract

We studied the properties and proper motions of Ellerman bombs (EBs) around a sunspot in a mature active region using high-resolution off-band Hα filtergrams together with nearly simultaneous magnetograms. Sixty-four percent of the EBs (class I) did not correspond accurately to enhanced magnetic field elements while the rest corresponded well to such elements (class II), which all were moving magnetic features (MMFs). We studied the lifetimes, shapes and dimensions, contrasts and time profiles of the EBs. These properties were essentially the same for both classes, in agreement with previous authors. Class I EBs did not move but class II EBs tracked the MMFs well, with horizontal proper motions up to a maximum of 1.1 km s^(−1) and their velocity pattern was similar to the velocity pattern of the MMFs.

Additional Information

© Kluwer Academic Publishers 1998. We would like to thank the staff of the Big Bear Solar Observatory for their support. This work was supported by NASA grants NAG5–2782 and NAGW–1972 and NSF grant ATM–9525971. AN would like to thank Dr S. M. White for useful discussions.

Additional details

Identifiers

Eprint ID
76415
DOI
10.1023/A:1005041920869
Resolver ID
CaltechAUTHORS:20170409-063602293

Funding

NASA
NAG5–2782
NASA
NAGW–1972
NSF
ATM–9525971

Dates

Created
2018-04-02
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Updated
2021-11-15
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