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Occurrence of Mesospheric Frontal Structures Over the High Latitude Station, Tromsø, Norway

JGR:Space physics - Thu, 07/11/2024 - 07:00
Abstract

Observational data sets for the high latitude middle atmosphere are key to understand the dynamics over those latitudes and the coupling between the lower and middle atmosphere. Utilizing long-term data sets from an all-sky imager at Tromsø, Norway (69.6°N, 19.2°E), the characteristics of 18 mesospheric frontal events in the Arctic winter mesosphere from 2011 to 2015 were studied. These frontal events exhibit horizontal extensions exceeding 500 km and were characterized by a sharp leading front, sometimes followed by a quasi-monochromatic wave train or a turbulent region. A subset of these frontal gravity wave events has been identified in the past as “bores.” While there have been numerous previous reports from low- and mid-latitude sites, and also from southern high latitudes, there have been a few from northern high latitudes. This study focuses on the frontal events in the northern high latitudes and provides new insights into the characteristics of these events. Their horizontal wavelengths primarily ranged from 20 to 40 km, and they exhibited phase speeds in the range 30–80 m/s. Most events were observed before local midnight. No clear link between these events and auroral activity was found. The majority of fronts were found propagating in the north-west direction, which might be due to the wind filtering effects.

Competing Influences of Earthward Convection and Azimuthal Drift Loss on the Pitch Angle Distribution of Energetic Electrons

JGR:Space physics - Thu, 07/11/2024 - 07:00
Abstract

Utilizing the multi-point observations by Van Allen Probe A, GOES 13 and 15, we analyzed the competing influences of earthward convection and azimuthal drift loss on the pitch angle distributions of energetic electrons during the simultaneous increases in solar wind flow velocity and pressure. The increase in solar wind speed amplifies the dawn-dusk convection electric field and causes the earthward transport of energetic electrons, and meanwhile the enhancement of solar wind dynamic pressure causes the inward displacement of dayside magnetopause and triggers the azimuthal drift loss of energetic electrons. The earthward convection of low-energy electrons (<60 keV) is much faster than their azimuthal drift loss at most pitch angles, and the fast earthward convections make the butterfly-like electron pitch angle distributions formed early become pancake-like distributions. The 60–530 keV electrons maintain the butterfly-like pitch angle distributions during the earthward convections, whereas the high-energy electrons above 530 keV are not transported to the low-L shells because of fast drift loss in the high-L source region. The competition between the earthward convection and the azimuthal drift loss finally determines the pitch angle distributions of energetic electrons near the trapping boundary during the increases in solar wind flow speed and pressure.

A physician’s legacy

Science - Thu, 07/11/2024 - 05:58
Science, Volume 385, Issue 6705, Page 149-149, July 2024.

Meet the Mississippi

Science - Thu, 07/11/2024 - 05:58
Science, Volume 385, Issue 6705, Page 148-148, July 2024.

Structured electrons with chiral mass and charge

Science - Thu, 07/11/2024 - 05:58
Science, Volume 385, Issue 6705, Page 183-187, July 2024.

Opening up

Science - Thu, 07/11/2024 - 05:58
Science, Volume 385, Issue 6705, Page 226-226, July 2024.

In Other Journals

Science - Thu, 07/11/2024 - 05:58
Science, Volume 385, Issue 6705, Page 155-156, July 2024.

Particle resupply in the lower atmosphere

Science - Thu, 07/11/2024 - 05:58
Science, Volume 385, Issue 6705, Page 144-144, July 2024.

Adaptive fungal invasion of bat cells

Science - Thu, 07/11/2024 - 05:58
Science, Volume 385, Issue 6705, Page 142-143, July 2024.

Sound evidence for biodiversity monitoring

Science - Thu, 07/11/2024 - 05:58
Science, Volume 385, Issue 6705, Page 138-140, July 2024.

Unmasking immune suppression

Science - Thu, 07/11/2024 - 05:58
Science, Volume 385, Issue 6705, Page 140-142, July 2024.

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