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Table 2

Geometry of the coma features found with image-enhancing techniques.

Date Feature PA − FWHMLS   (°) PA − FWHMAL   (°) PA   (°)

Feb. 9 A 64 – 8 A + B: 79 – 37 290
B 82 – 12
C 102 – 2 102 – 2
T 289 – 7 289 – 4

Mar. 10 SA 70 – 30 70 – 24 284
T 280 – 29 280 – 24

Mar. 22 SA 66 – 32 69 – 40 280
T 266 – 43 266 – 27

Apr. 22 AA 56 – 14 nd 193
SA 265 – 34 266 – 21
T nd nd

May 3 AA 73 – 23 nd 143
SA 267 – 19 268 – 22
T 136 – 19 nd

May 10 AA 60 – 19 nd 131
SA 269 – 25 267 – 28
T 138 – 24 nd

Jun. 15 SA 270 – 47 271 – 30 114
T 117 – 44 114 – 23

Jun. 16 SA 272 – 28 271 – 33 114
T 120 – 33 116 – 26

Jul. 3 SA 268 – 34 270 – 22 111
T 115 – 36 116 – 23

Aug. 4 SA 265 – 33 266 – 34 106
T 106 – 23 103 – 21

Sep. 9 SA 265 – 26 260 – 28 101
T 93 – 31 95 – 36

Notes. PA and FWHM are the position angle counted counterclockwise (east) from the north celestial pole and the width of the different coma features found with Larson-Sekanina (LS) and adaptive Laplace (AL) image-enhancing techniques, respectively. PA is the position angle of the extended Sun-target radius vector as seen in the observer’s plane-of-sky. nd stands for “not detected”.

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