Formation of Jet-driven Forced Reconnection Region and Associated Plasma Blobs in a Prominence Segment Article Swipe
Sudheer K. Mishra
,
A. K. Srivastava
,
S. P. Rajaguru
,
P. Jelínek
·
YOU?
·
· 2025
· Open Access
·
· DOI: https://doi.org/10.3847/1538-4357/adb8db
YOU?
·
· 2025
· Open Access
·
· DOI: https://doi.org/10.3847/1538-4357/adb8db
We use data from the Atmospheric Imaging Assembly on board the Solar Dynamics Observatory to study the most likely formation of a forced reconnection region and associated plasma blobs, triggered by jetlike structures in a prominence segment. Around 05:44 UT on 2017 December 16th, hot jetlike structures lifted from a nearby active region and fell obliquely on one side of the prominence segment with velocities of ≈45–65 km s −1 . These eruptions compressed the boundaries of the prominence and flux rope, forming an elongated reconnection region with inflow velocities of 47–52 km s −1 and 36–49 km s −1 in the projected plane. A thin, elongated reconnection region was formed, with multiple magnetic plasma blobs propagating bidirectionally at velocities of 91–178 km s −1 . These dense blobs, associated with ongoing reconnection, may also be linked to the onset of Kelvin–Helmholtz (K-H) instability. The blobs are attributed to plasmoids, moving at slower speeds (91–178 km s −1 ) due to the high density in the prominence segment. The dimensionless reconnection rate varied from 0.57–0.28, 0.53–0.26, and 0.41–0.20, indicating reconnection rate enhancement and supporting the forced reconnection scenario. After reconnection, the prominence plasma heated to 6 MK, releasing significant thermal energy (≈5.4 × 10 27 erg), which drained cool prominence plasma and heated it to coronal temperatures. The ubiquity of jets and outflows in the solar atmosphere makes the aforementioned reconnection and possible coexistence of K-H instability potentially important for the magnetic energy release and heating in the solar atmosphere.
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- Type
- article
- Language
- en
- Landing Page
- https://doi.org/10.3847/1538-4357/adb8db
- OA Status
- gold
- Cited By
- 1
- References
- 143
- Related Works
- 10
- OpenAlex ID
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All OpenAlex metadata
Raw OpenAlex JSON
- OpenAlex ID
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https://openalex.org/W4408875781Canonical identifier for this work in OpenAlex
- DOI
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https://doi.org/10.3847/1538-4357/adb8dbDigital Object Identifier
- Title
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Formation of Jet-driven Forced Reconnection Region and Associated Plasma Blobs in a Prominence SegmentWork title
- Type
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articleOpenAlex work type
- Language
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enPrimary language
- Publication year
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2025Year of publication
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2025-03-26Full publication date if available
- Authors
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Sudheer K. Mishra, A. K. Srivastava, S. P. Rajaguru, P. JelínekList of authors in order
- Landing page
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https://doi.org/10.3847/1538-4357/adb8dbPublisher landing page
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YesWhether a free full text is available
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goldOpen access status per OpenAlex
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https://doi.org/10.3847/1538-4357/adb8dbDirect OA link when available
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Physics, Jet (fluid), Plasma, Astrophysics, Magnetic reconnection, Astronomy, Mechanics, Nuclear physicsTop concepts (fields/topics) attached by OpenAlex
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1Total citation count in OpenAlex
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2025: 1Per-year citation counts (last 5 years)
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143Number of works referenced by this work
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10Other works algorithmically related by OpenAlex
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| abstract_inverted_index.of | 21, 60, 66, 77, 91, 121, 141, 220, 235 |
| abstract_inverted_index.on | 9, 41, 57 |
| abstract_inverted_index.to | 15, 138, 149, 161, 195, 215 |
| abstract_inverted_index.× | 203 |
| abstract_inverted_index.K-H | 236 |
| abstract_inverted_index.MK, | 197 |
| abstract_inverted_index.The | 145, 169, 218 |
| abstract_inverted_index.and | 26, 54, 80, 96, 177, 183, 212, 222, 232, 245 |
| abstract_inverted_index.are | 147 |
| abstract_inverted_index.due | 160 |
| abstract_inverted_index.for | 240 |
| abstract_inverted_index.hot | 45 |
| abstract_inverted_index.may | 134 |
| abstract_inverted_index.one | 58 |
| abstract_inverted_index.the | 5, 11, 17, 61, 75, 78, 102, 139, 162, 166, 185, 191, 225, 229, 241, 248 |
| abstract_inverted_index.use | 2 |
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| abstract_inverted_index.2017 | 42 |
| abstract_inverted_index.also | 135 |
| abstract_inverted_index.cool | 209 |
| abstract_inverted_index.data | 3 |
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| abstract_inverted_index.flux | 81 |
| abstract_inverted_index.from | 4, 49, 174 |
| abstract_inverted_index.high | 163 |
| abstract_inverted_index.jets | 221 |
| abstract_inverted_index.most | 18 |
| abstract_inverted_index.rate | 172, 181 |
| abstract_inverted_index.side | 59 |
| abstract_inverted_index.with | 64, 88, 112, 131 |
| abstract_inverted_index.−1 | 70, 95, 100, 125, 158 |
| abstract_inverted_index.(K-H) | 143 |
| abstract_inverted_index.05:44 | 39 |
| abstract_inverted_index.16th, | 44 |
| abstract_inverted_index.After | 189 |
| abstract_inverted_index.Solar | 12 |
| abstract_inverted_index.These | 72, 127 |
| abstract_inverted_index.blobs | 116, 146 |
| abstract_inverted_index.board | 10 |
| abstract_inverted_index.dense | 128 |
| abstract_inverted_index.erg), | 206 |
| abstract_inverted_index.makes | 228 |
| abstract_inverted_index.onset | 140 |
| abstract_inverted_index.rope, | 82 |
| abstract_inverted_index.solar | 226, 249 |
| abstract_inverted_index.study | 16 |
| abstract_inverted_index.thin, | 106 |
| abstract_inverted_index.which | 207 |
| abstract_inverted_index.Around | 38 |
| abstract_inverted_index.active | 52 |
| abstract_inverted_index.blobs, | 29, 129 |
| abstract_inverted_index.energy | 201, 243 |
| abstract_inverted_index.forced | 23, 186 |
| abstract_inverted_index.heated | 194, 213 |
| abstract_inverted_index.inflow | 89 |
| abstract_inverted_index.lifted | 48 |
| abstract_inverted_index.likely | 19 |
| abstract_inverted_index.linked | 137 |
| abstract_inverted_index.moving | 151 |
| abstract_inverted_index.nearby | 51 |
| abstract_inverted_index.plane. | 104 |
| abstract_inverted_index.plasma | 28, 115, 193, 211 |
| abstract_inverted_index.region | 25, 53, 87, 109 |
| abstract_inverted_index.slower | 153 |
| abstract_inverted_index.speeds | 154 |
| abstract_inverted_index.varied | 173 |
| abstract_inverted_index.(≈5.4 | 202 |
| abstract_inverted_index.36–49 | 97 |
| abstract_inverted_index.47–52 | 92 |
| abstract_inverted_index.Imaging | 7 |
| abstract_inverted_index.coronal | 216 |
| abstract_inverted_index.density | 164 |
| abstract_inverted_index.drained | 208 |
| abstract_inverted_index.formed, | 111 |
| abstract_inverted_index.forming | 83 |
| abstract_inverted_index.heating | 246 |
| abstract_inverted_index.jetlike | 32, 46 |
| abstract_inverted_index.ongoing | 132 |
| abstract_inverted_index.release | 244 |
| abstract_inverted_index.segment | 63 |
| abstract_inverted_index.thermal | 200 |
| abstract_inverted_index.91–178 | 122 |
| abstract_inverted_index.Abstract | 0 |
| abstract_inverted_index.Assembly | 8 |
| abstract_inverted_index.December | 43 |
| abstract_inverted_index.Dynamics | 13 |
| abstract_inverted_index.magnetic | 114, 242 |
| abstract_inverted_index.multiple | 113 |
| abstract_inverted_index.outflows | 223 |
| abstract_inverted_index.possible | 233 |
| abstract_inverted_index.segment. | 37, 168 |
| abstract_inverted_index.ubiquity | 219 |
| abstract_inverted_index.(91–178 | 155 |
| abstract_inverted_index.elongated | 85, 107 |
| abstract_inverted_index.eruptions | 73 |
| abstract_inverted_index.formation | 20 |
| abstract_inverted_index.important | 239 |
| abstract_inverted_index.obliquely | 56 |
| abstract_inverted_index.projected | 103 |
| abstract_inverted_index.releasing | 198 |
| abstract_inverted_index.scenario. | 188 |
| abstract_inverted_index.triggered | 30 |
| abstract_inverted_index.associated | 27, 130 |
| abstract_inverted_index.atmosphere | 227 |
| abstract_inverted_index.attributed | 148 |
| abstract_inverted_index.boundaries | 76 |
| abstract_inverted_index.compressed | 74 |
| abstract_inverted_index.indicating | 179 |
| abstract_inverted_index.plasmoids, | 150 |
| abstract_inverted_index.prominence | 36, 62, 79, 167, 192, 210 |
| abstract_inverted_index.structures | 33, 47 |
| abstract_inverted_index.supporting | 184 |
| abstract_inverted_index.velocities | 65, 90, 120 |
| abstract_inverted_index.≈45–65 | 67 |
| abstract_inverted_index.Atmospheric | 6 |
| abstract_inverted_index.Observatory | 14 |
| abstract_inverted_index.atmosphere. | 250 |
| abstract_inverted_index.coexistence | 234 |
| abstract_inverted_index.enhancement | 182 |
| abstract_inverted_index.instability | 237 |
| abstract_inverted_index.potentially | 238 |
| abstract_inverted_index.propagating | 117 |
| abstract_inverted_index.significant | 199 |
| abstract_inverted_index.0.41–0.20, | 178 |
| abstract_inverted_index.0.53–0.26, | 176 |
| abstract_inverted_index.0.57–0.28, | 175 |
| abstract_inverted_index.instability. | 144 |
| abstract_inverted_index.reconnection | 24, 86, 108, 171, 180, 187, 231 |
| abstract_inverted_index.dimensionless | 170 |
| abstract_inverted_index.reconnection, | 133, 190 |
| abstract_inverted_index.temperatures. | 217 |
| abstract_inverted_index.aforementioned | 230 |
| abstract_inverted_index.bidirectionally | 118 |
| abstract_inverted_index.Kelvin–Helmholtz | 142 |
| cited_by_percentile_year.max | 95 |
| cited_by_percentile_year.min | 91 |
| countries_distinct_count | 0 |
| institutions_distinct_count | 4 |
| citation_normalized_percentile.value | 0.8436782 |
| citation_normalized_percentile.is_in_top_1_percent | False |
| citation_normalized_percentile.is_in_top_10_percent | True |