Abstract
We report short-time variations in the plasma tail of C/2013 R1(Lovejoy). A series of short (2-3 minutes) exposure images with the 8.2 m Subaru telescope shows faint details of filaments and their motions over a 24 minute observing duration. We identified rapid movements of two knots in the plasma tail near the nucleus (∼3 × 105 km). Their speeds are 20 and 25 km s-1 along the tail and 3.8 and 2.2 km s-1 across it, respectively. These measurements set a constraint on an acceleration model of plasma tail and knots as they set the initial speed just after their formation. We also found a rapid narrowing of the tail. After correcting the motion along the tail, the narrowing speed is estimated to be ∼8 km s-1. These rapid motions suggest the need for high time-resolution studies of comet plasma tails with a large telescope.
| Original language | English |
|---|---|
| Article number | 97 |
| Journal | Astronomical Journal |
| Volume | 149 |
| Issue number | 3 |
| DOIs | |
| State | Published - Mar 1 2015 |
Keywords
- comets: individual (C/2013 R1)
- solar wind
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