dorsal/arxiv
View SchemaModeling Cosmogenic 10Be During the Heliosphere's Encounter with an Interstellar Cold Cloud
| Authors | Anna Nica, Merav Opher, Jesse Miller, Jennifer L. Middleton |
|---|---|
| Categories | |
| ArXiv ID | 2601.07983vv1 |
| URL | https://arxiv.org/abs/2601.07983 |
| License | http://creativecommons.org/licenses/by/4.0/ |
Abstract
Geologic records of cosmogenic 10Be are sensitive to changes in the radiation environment with time. Recent works suggest there are periods when the Sun encountered massive cold clouds which compressed the heliosphere to within Earth's orbit. This would expose Earth to increased galactic cosmic rays and MeV-energy particles of heliospheric origin. We model 10Be production in Earth's atmosphere during possible cold cloud encounters, and estimate their detectability in marine records of variable temporal resolution. We find that an AU-scale cold cloud encounter can be detected using ocean sediment measurements of 10Be if Earth spends time inside the compressed heliosphere. For typical relative speeds between the Sun and local interstellar clouds, this translates to a crossing time of ~100 years. A cloud must have an extension on the scale of parsecs to tens-of-parsecs (crossing time 0.1-1 Myr) to be detectable through 10Be measurements in iron-manganese crusts.
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"abstract": "Geologic records of cosmogenic 10Be are sensitive to changes in the radiation environment with time. Recent works suggest there are periods when the Sun encountered massive cold clouds which compressed the heliosphere to within Earth\u0027s orbit. This would expose Earth to increased galactic cosmic rays and MeV-energy particles of heliospheric origin. We model 10Be production in Earth\u0027s atmosphere during possible cold cloud encounters, and estimate their detectability in marine records of variable temporal resolution. We find that an AU-scale cold cloud encounter can be detected using ocean sediment measurements of 10Be if Earth spends time inside the compressed heliosphere. For typical relative speeds between the Sun and local interstellar clouds, this translates to a crossing time of ~100 years. A cloud must have an extension on the scale of parsecs to tens-of-parsecs (crossing time 0.1-1 Myr) to be detectable through 10Be measurements in iron-manganese crusts.",
"arxiv_id": "2601.07983",
"authors": [
"Anna Nica",
"Merav Opher",
"Jesse Miller",
"Jennifer L. Middleton"
],
"categories": [
"astro-ph.EP",
"astro-ph.GA",
"physics.ao-ph"
],
"license": "http://creativecommons.org/licenses/by/4.0/",
"title": "Modeling Cosmogenic 10Be During the Heliosphere\u0027s Encounter with an Interstellar Cold Cloud",
"url": "https://arxiv.org/abs/2601.07983",
"version": "v1"
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