Tuesday, September 30, 2025

How will a government shutdown affect NASA? | Rubin Observatory gets an algorithm update

Tumbleweed rovers may roll across Mars | Hubble Telescope quiz
Created for znamenski.spacecom@blogger.com | Web Version
 
September 30, 2025
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Happy Tuesday space fans!
Our newsroom is buzzing this morning with lots of headlines for your daily read, beginning with how a government shutdown will affect NASA, from astronauts on the ISS to future missions to Mars.

Other stories for today include a new algorithm that should improve the Rubin's Observatory images, SpaceX targeting October 13 for the next Starship launch and International Observe the Moon Day 2025 coming on October 4.

It's also Trivia Tuesday and our quiz for the week is all about the Hubble Space Telescope. We have all that and more for your newsletter.

Keep looking up,
Kenna
Content Manager, Space.com
 
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The algorithm models the blurring incurred by Earth's atmosphere and counteracts it, producing sharp and clear images.
 
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"The exploration of the moon is going to be a continuous activity."
 
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SpaceX
 
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Flight 11 will be the last launch of Starship's current "Version 2" iteration.
 
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Technology
 
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Seminars Digest, Vol 77, Issue 8

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1. Friday 03.10.2025 (info+seminars@itp.ac.ru)


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Message: 1
Date: Tue, 30 Sep 2025 07:02:02 +0000
From: info+seminars@itp.ac.ru
To: staff@itp.ac.ru, students@itp.ac.ru, seminars@itp.ac.ru
Subject: [Landau ITP Seminars] Friday 03.10.2025
Message-ID: <6i75AoIK6iyduqCpFerkIx4gDMp0M8BySggSivd3w0k@wwwserv2>
Content-Type: text/plain; charset=UTF-8

Уважаемые коллеги!

На заседании Ученого совета ИТФ в пятницу 03.10 будет заслушан 1 доклад:
11:30 M. A. Skvortsov, A. V. Polkin
Thermal phase slips in superconducting films and Boussinesq equation

A dissipationless supercurrent state in superconductors can be destroyed by thermal fluctuations. Thermally activated phase slips provide a finite resistance of the sample and are responsible for dark counts in superconducting single photon detectors. The activation barrier for a phase slip is determined by a space-dependent saddle-point (instanton) configuration of the order parameter. In the one-dimensional wire geometry, such a saddle point has been analytically obtained by Langer and Ambegaokar in the vicinity of the critical temperature, $T_c$, and for arbitrary bias currents below the critical current $I_c$. In the two-dimensional geometry of a superconducting strip, which is relevant for photon detection, the situation is much more complicated. Depending on the ratio $I/I_c$, several types of saddle-point configurations have been proposed, with their energies being obtained numerically. We demonstrate that the saddle-point configuration for an infinite superconducting film at $I\to I_c$ is described by the exactly integrable Boussinesq equation solved by Hirota&#039;s method. The instanton size is $L_x\sim\xi(1-I/I_c)^{-1/4}$ along the current and $L_y\sim\xi(1-I/I_c)^{-1/2}$ perpendicular to the current, where $\xi$ is the Ginzburg-Landau coherence length. The activation energy for thermal phase slips scales as $\Delta F^\text{2D}\propto (1-I/I_c)^{3/4}$. For sufficiently wide strips of width $w\gg L_y$, a half-instanton is formed near the boundary, with the activation energy being 1/2 of $\Delta F^\text{2D}$.

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