The first simultaneous spectroscopic and monochromatic imaging observations of short-wavelength infrared aurora of N2+ Meinel (0,0) band at 1.1 μm with incoherent scatter radar

被引:0
作者
Nishiyama, Takanori [1 ,2 ]
Kagitani, Masato [3 ]
Furutachi, Senri [4 ]
Iwasa, Yuki [5 ]
Ogawa, Yasunobu [1 ,2 ]
Tsuda, Takuo T. [4 ]
Dalin, Peter [6 ]
Tsuchiya, Fuminori [3 ]
Nozawa, Satonori [7 ]
Sigernes, Fred [8 ]
机构
[1] Natl Inst Polar Res, 10-3 Midori Cho, Tokyo 1908518, Japan
[2] SOKENDAI, Dept Polar Sci, Grad Univ Adv Studies, 10-3 Midori Cho, Tokyo 1908518, Japan
[3] Tohoku Univ, 6-3,Aramaki Aza Aoba,Aoba Ku, Sendai, Miyagi 9808578, Japan
[4] Univ Electrocommun, Dept Comp & Network Engn, 1-5-1 Chofugaoka, Tokyo 1828585, Japan
[5] Natl Inst Adv Ind Sci & Technol, NMIJ, 1-1-1 Umezono, Tsukuba, Ibaraki 3058563, Japan
[6] Swedish Inst Space Phys, Box 812, SE-98128 Kiruna, Sweden
[7] Nagoya Univ, Inst Space Earth Environm Res, Furo Cho,Chikusa Ku, Nagoya, Aichi 4648601, Japan
[8] Univ Ctr Svalbard, Longyearbyen, Norway
来源
EARTH PLANETS AND SPACE | 2024年 / 76卷 / 01期
基金
日本学术振兴会;
关键词
Aurora; Short-wavelength infrared; Ground-based spectroscopic observations; Ground-based imaging; Indium gallium arsenide; Polar cap; Incoherent scatter radar; Kjell Henriksen Observatory; QUANTITATIVE SPECTROSCOPY; SPECTRUM;
D O I
10.1186/s40623-024-01969-x
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
This study presents a first simultaneous observation of N-2(+) Meinel (0,0) band (hereafter, N-2(+) (M)) aurora by cutting-edge short-wavelength infrared imaging spectrograph (NIRAS-2) and monochromatic camera (NIRAC) installed at the Kjell Henriksen Observatory (78 degrees N, 16 degrees E). On January 21 2023, N-2(+) (M) intensification that is associated with a band-shape aurora structure was observed by the NIRAS-2 and the NIRAC having temporal resolutions of 30 s and 20 s, respectively. In addition, the European incoherent scatter Svalbard Radar also observed electron density variations at the same time. Electron density measured at altitude range from 100 km 120 km shows similar variations as of N-2(+) (M) intensity, which implies that a primary source of N-2(+) (M) emissions is direct collisions of N-2 by precipitating electrons penetrating down to around 100 km altitude (up to 10 keV). However, the observation also demonstrated moderate correlations between N-2(+) (M) intensity and electron density above 140 km, which implies that different N-2(+) (M) generation process, N-2 charge exchange with O+, may work up to near 160 km and make a non-negligible contribution to N-2(+) (M) emissions. This hypothesis would be verified with further radar observations or stereo imaging observations useful to estimate the vertical distribution of the emission layers. The N-2(+) (M) is a very promising target wavelength for aurora observation because the quality of sensors is highly expected to improve further and further. Continuous observations with our new instruments will undoubtedly provide an important information of N-2(+) (M) characteristics, for future missions of both balloon-borne and satellite-borne imaging.
引用
收藏
页数:9
相关论文
共 18 条
  • [1] The Space Physics Environment Data Analysis System (SPEDAS)
    Angelopoulos, V.
    Cruce, P.
    Drozdov, A.
    Grimes, E. W.
    Hatzigeorgiu, N.
    King, D. A.
    Larson, D.
    Lewis, J. W.
    McTiernan, J. M.
    Roberts, D. A.
    Russell, C. L.
    Hori, T.
    Kasahara, Y.
    Kumamoto, A.
    Matsuoka, A.
    Miyashita, Y.
    Miyoshi, Y.
    Shinohara, I.
    Teramoto, M.
    Faden, J. B.
    Halford, A. J.
    McCarthy, M.
    Millan, R. M.
    Sample, J. G.
    Smith, D. M.
    Woodger, L. A.
    Masson, A.
    Narock, A. A.
    Asamura, K.
    Chang, T. F.
    Chiang, C. -Y.
    Kazama, Y.
    Keika, K.
    Matsuda, S.
    Segawa, T.
    Seki, K.
    Shoji, M.
    Tam, S. W. Y.
    Umemura, N.
    Wang, B. -J.
    Wang, S. -Y.
    Redmon, R.
    Rodriguez, J. V.
    Singer, H. J.
    Vandegriff, J.
    Abe, S.
    Nose, M.
    Shinbori, A.
    Tanaka, Y. -M.
    UeNo, S.
    [J]. SPACE SCIENCE REVIEWS, 2019, 215 (01)
  • [2] VIBRATIONAL DEVELOPMENT OF THE N-2+ MEINEL BAND SYSTEM IN THE AURORA
    ESPY, PJ
    PENDLETON, WR
    SIVJEE, GG
    FETROW, MP
    [J]. JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1987, 92 (A10): : 11257 - 11261
  • [3] QUANTITATIVE SPECTROSCOPY OF THE AURORA .5. THE SPECTRUM OF STRONG AURORA BETWEEN 10000-A AND 16000-A
    GATTINGER, RL
    JONES, AV
    [J]. CANADIAN JOURNAL OF PHYSICS, 1981, 59 (03) : 480 - 487
  • [4] N2+ MEINEL AURORAL SPECTRA IN 1.5 MU REGION
    GATTINGER, RL
    JONES, AV
    [J]. CANADIAN JOURNAL OF PHYSICS, 1973, 51 (03) : 287 - 291
  • [5] Harrison AW., 1957, region J, DOI [10.1016/0021-9169(57)90065-X, DOI 10.1016/0021-9169(57)90065-X]
  • [6] QUANTITATIVE SPECTROSCOPY OF AURORA .4. SPECTRUM OF MEDIUM INTENSITY AURORA BETWEEN 8800-A AND 11 400-A
    JONES, AV
    GATTINGER, RL
    [J]. CANADIAN JOURNAL OF PHYSICS, 1976, 54 (21) : 2128 - 2133
  • [7] THE AURORAL SPECTRUM FROM 6200-A TO 8900-A
    MEINEL, AB
    [J]. ASTROPHYSICAL JOURNAL, 1951, 113 (03) : 583 - &
  • [8] Nishiyama T, 2021, EARTH PLANETS SPACE, V73, DOI 10.1186/s40623-021-01360-0
  • [9] THE RED AND NEAR-INFRA-RED AURORAL SPECTRUM
    OMHOLT, A
    [J]. JOURNAL OF ATMOSPHERIC AND TERRESTRIAL PHYSICS, 1957, 10 (5-6): : 320 - &
  • [10] First ground-based measurements of OI 6300 Å daytime aurora over Boston in response to the 30 October 2003 geomagnetic storm -: art. no. L03S10
    Pallamraju, D
    Chakrabarti, S
    [J]. GEOPHYSICAL RESEARCH LETTERS, 2005, 32 (03) : 1 - 4