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ALMA observations of transient heating in a solar active region

da Silva Santos, João Manuel (author)
Stockholms universitet,Institutionen för astronomi
de la Cruz Rodríguez, Jaime (author)
Stockholms universitet,Institutionen för astronomi
White, Stephen M. (author)
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Leenaarts, Jorrit (author)
Stockholms universitet,Institutionen för astronomi
Vissers, Gregal J. M. (author)
Stockholms universitet,Institutionen för astronomi
Hansteen, Viggo H. (author)
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 (creator_code:org_t)
2020-10-29
2020
English.
In: Astronomy and Astrophysics. - : EDP Sciences. - 0004-6361 .- 1432-0746. ; 643
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • Aims. We aim to investigate the temperature enhancements and formation heights of solar active-region brightenings such as Ellerman bombs (EBs), ultraviolet bursts (UVBs), and flaring active-region fibrils (FAFs) using interferometric observations in the millimeter (mm) continuum provided by the Atacama Large Millimeter/submillimeter Array (ALMA).Methods. We examined 3 mm signatures of heating events identified in Solar Dynamics Observatory observations of an active region and compared the results with synthetic spectra from a 3D radiative magnetohydrodynamic simulation. We estimated the contribution from the corona to the mm brightness using differential emission measure analysis.Results. We report the null detection of EBs in the 3 mm continuum at ∼1.2″ spatial resolution, which is evidence that they are sub-canopy events that do not significantly contribute to heating the upper chromosphere. In contrast, we find the active region to be populated with multiple compact, bright, flickering mm-bursts – reminiscent of UVBs. The high brightness temperatures of up to ∼14 200 K in some events have a contribution (up to ∼7%) from the corona. We also detect FAF-like events in the 3 mm continuum. These events show rapid motions of > 10 kK plasma launched with high plane-of-sky velocities (37 − 340 km s−1) from bright kernels. The mm FAFs are the brightest class of warm canopy fibrils that connect magnetic regions of opposite polarities. The simulation confirms that ALMA should be able to detect the mm counterparts of UVBs and small flares and thus provide a complementary diagnostic for localized heating in the solar chromosphere.

Subject headings

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

Keyword

Sun: atmosphere
Sun: chromosphere
Sun: corona
Sun: UV radiation
Sun: radio radiation
Sun: activity
Astronomy
astronomi

Publication and Content Type

ref (subject category)
art (subject category)

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