On the nighttime enhancement in ionospheric electron density over - - PowerPoint PPT Presentation

on the nighttime enhancement in ionospheric electron
SMART_READER_LITE
LIVE PREVIEW

On the nighttime enhancement in ionospheric electron density over - - PowerPoint PPT Presentation

On the nighttime enhancement in ionospheric electron density over the equatorial region Sneha Yadav, R. K. Choudhary, Surendra Sunda, P. R. Shreedevi, and T. K. Pant Space Physics Laboratory, Vikram Sarabhai Space Centre, Thiruvananthapuram,


slide-1
SLIDE 1

On the nighttime enhancement in ionospheric electron density over the equatorial region

Sneha Yadav, R. K. Choudhary, Surendra Sunda, P. R. Shreedevi, and T. K. Pant

Space Physics Laboratory, Vikram Sarabhai Space Centre, Thiruvananthapuram, India sneha.yadav84@gmail.com

May 21, 2019 ICTP, Trieste, Italy

slide-2
SLIDE 2

Ionospheric Nighttime Enhancement (INE)

“At nighttime, during the absence of ionization, the ionospheric electron density is generally expected to decay gradually but it does not behave as predicted by the simple notion and show enhancement occasionally”. This phenomenon is called ionospheric nighttime enhancement (INE).

  • Based on the time of occurrence, INEs have been classified into two types:

Premidnight and Postmidnight

  • According to the geographic region, they can be categorized as:

Mid-latitude, Low-latitude and Equatorial INEs

  • The underlying physical mechanism proposed for different INE events are also

different.

  • The studies regarding INEs over the equatorial region are rather sparse.
slide-3
SLIDE 3

Equatorial and Low-Latitude Ionosphere

The unique configuration

  • f

geomagnetic field lines over the geomagnetic equator forms the base for the various plasma processes.

  • Equatorial Electrojet (EEJ),
  • Equatorial Ionization Anomaly

(EIA)

  • Equatorial Spread- F (ESF)

EIA Ionization crest Geomagnetic Field lines Ionization trough Irregularities

slide-4
SLIDE 4

Equatorial Ionization Anomaly

Watthanasangmechai et al., 2013 Basu et al., 2002

Reverse Fountain Effect: Consequence

  • f the change in the direction of the

zonal electric field from eastward to westward and characterized by the movement of the EIA crest towards the equator. Fountain effect: During the daytime, the eastward zonal electric field in conjunction with the horizontal N-S component of the geomagnetic field gives rise to the vertical E × B drift over the geomagnetic equator which in turn lifts the plasma to higher altitudes.

slide-5
SLIDE 5

GPS Aided Geo Augmented Navigation (GAGAN)

  • There are 15 reference stations under SBAS-GAGAN.
  • A unique iono model was developed for GAGAN to

broadcast the vertical delay (GIVD) at IGPs.

  • GAGAN is broadcasting the ionospheric corrections over

102 (IGP) ionospheric grid points (5° Lat x 5° Long) through Geostationary satellites.

A very simplistic and novel approach as suggested by

Sunda et al., [2015] has been used to generate the spatio- temporal TEC maps over the Indian region using GAGAN.

INDIAN SBAS

slide-6
SLIDE 6

16 March 2015 Quiet Day 17 March 2015 Geomagnetic storm day 18 March 2015 Recovery day

Yadav et al., 2016

GAGAN generated 2D-TEC Maps

slide-7
SLIDE 7

GPS measurements Trivandrum (8.5°N, 77.1°E, 0.5°N) Bengaluru (12.9°N, 77.6°E, 4.1°N)

Dataset

Ionosonde measurements over Trivandrum: foF2: F2 region critical frequency h’F: F-region base height hmF2: peak electron density height of the F2 region Vz: Vertical drift Satellite Based Augmentation System (SBAS): To study the motion of EIA Case Study Based on the common availability of the dataset Indian Space Weather Ionospheric Monitoring stations

slide-8
SLIDE 8

Typical Examples of INE

Trivandrum (8.5°N, 77.1°E, 0.5°N) Bangalore (12.9°N, 77.6°E, 4.1°N)

slide-9
SLIDE 9
  • The preceding minimum of electron

densities after sunset has been chosen as the reference to quantify the nighttime enhancement.

  • The TEC values are subtracted from this

reference level.

Night-time Enhancement Event Identification

slide-10
SLIDE 10

Typical Examples of INE

slide-11
SLIDE 11

CASE1: 01 Feb 2014

  • The two humps in the ΔTEC values
  • ver both the station is well

discernible from the figure.

  • The enhancement in the

postmidnight ΔTEC values appears first over Bangalore and then over Trivandrum.

  • The vertical drift remains westward

from ~16 to 19 UT with a maximum value of -25m/s.

slide-12
SLIDE 12

Motion of EIA during Night-time over the Indian longitudes

CASE1: 01 Feb 2014

SBAS 2D-TEC Maps

slide-13
SLIDE 13

CASE2: 21 Feb 2014

slide-14
SLIDE 14

CASE3: 06 Feb 2014

slide-15
SLIDE 15

CASE5: 20 Feb 2014

slide-16
SLIDE 16

Westward electric field Downward E × B drift Reverse plasma fountain Equatorward Meridional wind

Night-time Equatorial ionosphere

Transport higher- density plasma towards equator Increase in electron density over equator

Mechanism responsible for INE

slide-17
SLIDE 17

Summary

  • The GAGAN (Indian SBAS) generated maps are effective in studying in the

reverse fountain effect.

  • Results enable visualizing the association of mid-night enhancement in the

electron density over the equatorial region with the reverse fountain effect.

  • Results suggests that the combined effect of downward E × B plasma drift

due to westward electric field and equatorward meridional at night are the main driving force for the nighttime enhancement over equatorial regions.

Thank You !