Simultaneous observations for MLT Neutral Winds by FPI and Meteor - - PowerPoint PPT Presentation

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Simultaneous observations for MLT Neutral Winds by FPI and Meteor - - PowerPoint PPT Presentation

Simultaneous observations for MLT Neutral Winds by FPI and Meteor Radar at King Sejong Station(KSS), Antarctica: Brief report Geonhwa Jee , Changsup Lee, Jeong-Han Kim Korea Polar Research Institute (KOPRI), Incheon, Korea Won-Seok Lee, Yongha Kim


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Simultaneous observations for MLT Neutral Winds by FPI and Meteor Radar at King Sejong Station(KSS), Antarctica: Brief report

Geonhwa Jee, Changsup Lee, Jeong-Han Kim

Korea Polar Research Institute (KOPRI), Incheon, Korea

Won-Seok Lee, Yongha Kim

Chungnam National University, Daejeon, Korea

Qian Wu

NCAR/HAO, Boulder, CO, USA

4th International ANGWIN workshop, INPE, São José dos Campos, SP , Brasil, 24-26 April 2018

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King Sejong Station (KSS)

Geomagnetic North Pole Dasan Station (& KHO)

78° 55' N, 11° 56' E

King Sejong Station (KSS)

62° 13' S, 58° 47' W

Jang Bogo Station (JBS)

74º 37' S, 164º 13' E

Kiruna (Esrange)

67° 51' N, 20° 13' E

Geomagnetic South Pole

Palmer

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Optical Obs. FPI & ASC Meteor Radar

King Sejong Station (KSS)

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KSS-Meteor Radar

Jang Bogo Station (JBS) Kiruna

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KSS-Meteor Radar

Jang Bogo Station (JBS) Kiruna

  • ATRAD meteor detection radar
  • Continuously operated since March 2007
  • Number of echo: 15,000~40,000 per day, which is more

than twice of typical meteor radar observations

  • Hourly mean neutral wind profiles (75~105 km) and daily

mean temperature at around the meteor peak height (~ 90 km)

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KSS-FPI

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KSS-FPI

  • It was operated by NCAR/HAO at US Palmer station,

Antarctica

  • Moved to KSS in Jan. 2017 in collaboration with NCAR/

HAO

  • Operates with three filters for 630.0 nm, 557.7 nm, 892.0

nm airglow emissions

  • Snapshot winds for each filter with about 55 min.

temporal resolution

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Spatial Coverage

75 km 105 km 250 km 87 km 97 km ~200 km meteor

  • bs.

892.0nm 557.7nm

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FPI vs. MR

FPI winds MR winds Temporal resol.

55 min. (with 3 filters) :snap shot winds & temp. for each filter 1 hour :hourly mean winds & daily mean temp.

Spatial resol.

~200 km ~250 km

Height

87 km (OH 892.0 nm) 97 km (O 557.7 nm) 250 km (O 630.0 nm) 75~105 km (with 2 km step)

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FPI & MR : Meridional winds

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FPI & MR : Zonal winds

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→ : OI 5577(97 km) → : OH 8920(87 km) → : meteor radar(75 ~ 105km, 2km bin)

N S W E

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→ : OI 5577(97 km) → : OH 8920(87 km) → : meteor radar(75 ~ 105km, 2km bin)

N S W E

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→ : OI 5577(97 km) → : OH 8920(87 km) → : meteor radar(75 ~ 105km, 2km bin)

N S W E

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→ : OI 5577(97 km) → : OH 8920(87 km) → : meteor radar(75 ~ 105km, 2km bin)

N S W E

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Correlation btw MR and FPI winds

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FPI vs. MR winds at mid- latitude region

Yu et al., 2016

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Summary

  • Simultaneous measurements of MLT neutral winds at KSS, Antarctica.

However,

  • Optical vs. radar
  • Snapshot vs. hourly mean winds
  • Relatively large differences may indicate that there are large variabilities

within 1-hour time period in the MLT winds.

  • Any complementary aspects of these two measurements?
  • What information can we obtain with this simultaneous observation?
  • With the MR wind observations, is it necessary to keep observing the

MLT winds by FPI?

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Future works

  • Large number of observed meteor echos: 15,000~40,000

per day

  • Increase the temporal resolution of neutral wind
  • bservation: 1-hour —> 0.5-hour
  • Daily mean temperature —> separate day & night mean

temperatures

  • Compare them with FPI winds & temp.