Results 31 to 40 of about 4,597 (205)
Mercury's Exosphere as Seen by BepiColombo/PHEBUS Visible Channels During the First Two Flybys
Abstract BepiColombo, the ESA/JAXA joint mission performed its first flyby of Mercury on 1 October 2021 and its second on 23 June 2022. PHEBUS observed the exosphere of Mercury during these flybys notably with its visible channels c404 (centered on the potassium emission line at 404 nm) and c422 (centered on the calcium emission line at 422 nm).
R. Robidel +12 more
wiley +1 more source
A Dust Detection Database for the Inner Heliosphere Using the Parker Solar Probe Spacecraft
A database of in situ dust impact detections made by the Parker Solar Probe spacecraft is created to facilitate studies of interplanetary dust dynamics in the inner heliosphere.
David M. Malaspina +6 more
doaj +1 more source
PAWS and POCO: NIR Astrophotonic Instruments for Astronomy
Abstract For near‐infrared ground and space‐based astronomy, compact photonic devices can replace the large bulk optical components in spectrographs, frequency combs, beam combiners, and sky subtraction filters, thus saving cost, reducing volume, weight, and power requirements.
Kalaga Madhav +8 more
wiley +1 more source
Near-infrared Polarization Charateristics of the Zodiacal Light Observed with DIRBE/COBE
We report near-infrared polarization of the zodiacal light (ZL) measured from space by the Diffuse Infrared Background Experiment (DIRBE) on board the Cosmic Background Explorer in photometric bands centered at 1.25, 2.2, and 3.5 μ m.
Kohji Takimoto +3 more
doaj +1 more source
Decadal and Annual Variations in Meteoric Flux From Ulysses, Wind, and SOFIE Observations
Abstract Our solar system is filled with meteoric particles, or cosmic dust, which is either interplanetary or interstellar in origin. Interstellar dust (ISD) enters the heliosphere due to the relative motion of the sun and the interstellar flow. Interplanetary dust (IPD) comes primarily from asteroid collisions or comet sublimation, and comprises the ...
Mark E. Hervig +5 more
wiley +1 more source
Zodiacal Cloud Complexes [PDF]
We discuss some aspects of the study of the Zodiacal cloud based on brightness observations. The discussion of optical properties as well as the spatial distribution of the dust cloud show that the description of the dust cloud as a homogeneous cloud is reasonable for the regions near the Earth orbit, but fails in the description of the dust in the ...
openaire +2 more sources
Midnight Sun to Polar Night: A Model of Seasonal Light in the Barents Sea
Abstract Arctic marine ecosystems are strongly influenced by the extreme seasonality of light in the region. Accurate determination of light is essential for building a comprehensive understanding of the dynamics of animal and aquatic algae populations.
Stacey Connan‐McGinty +8 more
wiley +1 more source
The diffuse, unresolved sky provides most of the photons that the Hubble Space Telescope (HST) receives, yet remains poorly understood. The HST Archival Legacy program SKYSURF aims to measure the 0.2–1.6 μ m sky surface brightness (sky-SB) from over 140 ...
Rosalia O’Brien +24 more
doaj +1 more source
Whiting Events in a Large Peri‐Alpine Lake: Evidence of a Catchment‐Scale Process
Abstract Whiting events are transient phenomena commonly occurring in hardwater lakes and manifesting as a turquoise coloration of surface waters during massive calcium carbonate precipitation. While biological and physico‐chemical drivers of carbonate precipitation are known, their relative contributions in controlling whiting events' timing and ...
Nicolas Escoffier +7 more
wiley +1 more source
Mercury's Circumsolar Dust Ring as an Imprint of a Recent Impact
A circumsolar dust ring has been recently discovered close to the orbit of Mercury. There are currently no hypotheses for the origin of this ring in the literature, so we explore four different origin scenarios here: the dust originated from (1) the ...
Petr Pokorný +2 more
doaj +1 more source

