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| Content Provider | Springer Nature Link |
|---|---|
| Author | Zhang, Q. M. Ji, H. S. Su, Y. N. |
| Copyright Year | 2016 |
| Abstract | Coronal bright points (CBPs) and jets are ubiquitous small-scale brightenings that are often associated with each other. We here report our multiwavelength observations of two groups of homologous jets. The first group was observed by the Extreme-Ultraviolet Imager (EUVI) onboard the Solar TErrestrial RElations Observatory (STEREO) Behind spacecraft in 171 Å and 304 Å on 2014 September 10, from a location where no data from the Solar Dynamic Observatory (SDO) could be obtained. The jets (J1 – J6) recurred for six times with intervals of 5 – 15 minutes. They originated from the same primary CBP (BP1) and propagated in the northeast direction along large-scale, closed coronal loops. Two of the jets (J3 and J6) produced sympathetic CBPs (BP2 and BP3) after reaching the remote footpoints of the loops. The time delays between the peak times of BP1 and BP2 (BP3) are $240\pm75~\mbox{s}$ ( $300\pm75~\mbox{s}$ ). The jets were not coherent. Instead, they were composed of bright and compact blobs. The sizes and apparent velocities of the blobs are 4.5 – 9 Mm and 140 – 380 km s$^{−1}$. The arrival times of the multiple blobs in the jets at the far end of the loops indicate that the sympathetic CBPs are caused by jet flows and not by thermal conduction fronts. The second group was observed by the Atmospheric Imaging Assembly onboard SDO in various wavelengths on 2010 August 3. Similar to the first group, the jets originated from a short-lived BP at the boundary of Active Region 11092 and propagated along a small-scale, closed loop before flowing into the active region. Several tiny blobs with sizes of $\sim1.7~\mbox{Mm}$ and an apparent velocity of $\sim238~\mbox{km}\,\mbox{s}^{-1}$ were identified in the jets. We carried out differential emission measure (DEM) inversions to investigate the temperatures of the blobs, finding that the blobs were multithermal with an average temperature of 1.8 – 3.1 MK. The estimated number densities of the blobs were $(1.7\,\mbox{--}\,2.8)\times10^{9}~\mbox{cm}^{-3}$ . |
| Starting Page | 859 |
| Ending Page | 876 |
| Page Count | 18 |
| File Format | |
| ISSN | 00380938 |
| Journal | Solar Physics |
| Volume Number | 291 |
| Issue Number | 3 |
| e-ISSN | 1573093X |
| Language | English |
| Publisher | Springer Netherlands |
| Publisher Date | 2016-03-18 |
| Publisher Place | Dordrecht |
| Access Restriction | One Nation One Subscription (ONOS) |
| Subject Keyword | Flares, microflares and nanoflares Magnetic reconnection, observational signatures Jets Astrophysics and Astroparticles Atmospheric Sciences Extraterrestrial Physics, Space Sciences |
| Content Type | Text |
| Resource Type | Article |
| Subject | Astronomy and Astrophysics Space and Planetary Science |
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