「
Since We Use Non-linear Artificial Diffusion
」を編集中
2025年10月22日 (水) 01:21時点における
ChrisRiddoch97
(
トーク
|
投稿記録
)
による版
(
差分
)
← 古い版
|
最新版
(
差分
) |
新しい版 →
(
差分
)
ナビゲーションに移動
検索に移動
警告: このページの古い版を編集しています。
公開すると、この版以降になされた変更がすべて失われます。
警告:
ログインしていません。編集を行うと、あなたの IP アドレスが公開されます。
ログイン
または
アカウントを作成
すれば、あなたの編集はその利用者名とともに表示されるほか、その他の利点もあります。
スパム攻撃防止用のチェックです。 けっして、ここには、値の入力は
しない
でください!
<br>We perform an unprecedented excessive-decision simulation for the solar convection zone. Our calculation reproduces the fast equator and near-floor shear layer (NSSL) of differential rotation and the near-surface poleward meridional movement simultaneously. The NSSL is positioned in a posh layer where the spatial and time scales of thermal convection are considerably small in contrast with the deep convection zone. While there have been several attempts to reproduce the NSSL in numerical simulation, [https://thaprobaniannostalgia.com/index.php/Since_We_Use_Non-linear_Artificial_Diffusion Wood Ranger Power Shears] the results are still removed from actuality. On this examine, we succeed in reproducing an NSSL in our new calculation. 4) the turbulent viscosity and magnetic tension are latitudinally balanced with the Coriolis force in the NSSL. We emphasize the significance of the magnetic discipline within the photo voltaic convection zone. ††software: R2D2 Hotta et al. The Sun is rotating differentially with the fast equator and the gradual pole. Omega in the solar inside. In the photo voltaic convection zone, we have now two shear layers, i.e., the tachocline around the bottom of the convection zone and the close to-surface shear layer (NSSL).<br><br><br><br>The tachocline is thought to be maintained by the interaction between the convection and radiation zones (Spiegel & Zahn, 1992; Gough & McIntyre, 1998; Forgács-Dajka & Petrovay, 2001; Rempel, 2005; Brun et al., 2011; Matilsky et al., 2022). The NSSL is thought to be maintained by the small-spatial and [https://tiny-links.net/bernadinesperr Wood Ranger Power Shears manual] [https://git.dehemi.com/helenegrogan1 Wood Ranger Power Shears price] [https://digitalsnax.com/clairetonga472 electric power shears] [http://git.gkcorp.com.vn:16000/carrollbristow Wood Ranger Power Shears] sale quick time scales of the convection within the layer. T/g, the place TT and gg are the temperature and the gravitational acceleration, respectively. 60 and a pair of Mm, [http://wiki.konyvtar.veresegyhaz.hu/index.php?title=Discover_Precision_Cutting_With_Top-Quality_Fabric_Scissors Wood Ranger Power Shears] respectively. Thus, [http://www.onestopclean.kr/bbs/board.php?bo_table=free&wr_id=722289 Wood Ranger Power Shears] the time scales of the convection range from a month to a number of hours in these regions. In consequence, the convection within the NSSL is just not considerably affected by the rotation. ′ denote the longitudinal average and the deviation from the common. In addition, Miesch & Hindman (2011) counsel that we'd like a drive to stability with the latitudinal Coriolis force to take care of the NSSL. It is tough for numerical simulations to cover a broad range of spatial and time scales. The numerical strategy for the NSSL is extremely restricted.<br> <br><br><br>Guerrero et al. (2013) improve the superadiabaticity round the highest boundary of their calculation box and focus on the formation mechanism of the NSSL following Foukal & Jokipii (1975). Hotta et al. NSSL-like function, particularly at low and high latitudes. We argue there that the NSSL is maintained by the radially inward angular momentum transport and the turbulent viscosity on the sheared meridional move. Hotta et al. (2015) fail to reproduce the NSSL in mid-latitude. Matilsky et al. (2019) perform a similar calculation to Hotta et al. 2015) and reproduce the NSSL-like function at high and [https://source.yysfan.com/broderickponde Wood Ranger Power Shears] low latitudes. The authors also fail to reproduce the NSSL in the mid-latitude. They conclude that the detailed construction mechanism of the meridional circulation should be understood to reproduce the proper NSSL. In their study, extremely rotationally constrained convection known as the Busse column, is required to reproduce the photo voltaic-like fast equator differential rotation. Hotta et al. (2015) lowered the solar luminosity and Matilsky et al.<br><br><br><br>2019) increased the rotation rate in order to enhance the rotational affect on the thermal convection. We be aware that the decrease in luminosity and the rise in rotation fee have the same effect on the Rossby number. Matilsky et al. (2019) argue that when the rotationally constrained Busse column exists within the deep layer, [http://dogetransparency.wiki/index.php/User:EldonMagrath11 Wood Ranger Power Shears] upflows are rotationally constrained even in the close to-floor excessive Rossby quantity layer. The environment friendly generation of the near-surface circulation through the gyroscopic pumping successfully suppresses the development of the NSSL. When the previous calculation (Hotta et al., 2015; Matilsky et al., 2019) was carried out, we didn't have any way to keep up the solar-like DR without utilizing the lowered luminosity, larger rotation rates or enhanced diffusivities (solar convective conundrum). That's, the everyday "high-resolution" simulations fall into anti-photo voltaic differential rotation. O’Mara et al., 2016; Hotta et al., 2023). Hotta & Kusano (2021)(hereafter HK21) and Hotta et al. 2022)(hereafter HKS22) not too long ago present a potential answer to assemble the photo voltaic-like differential rotation with out utilizing special treatment shown above.<br>
編集内容の要約:
鈴木広大への投稿はすべて、他の投稿者によって編集、変更、除去される場合があります。 自分が書いたものが他の人に容赦なく編集されるのを望まない場合は、ここに投稿しないでください。
また、投稿するのは、自分で書いたものか、パブリック ドメインまたはそれに類するフリーな資料からの複製であることを約束してください(詳細は
鈴木広大:著作権
を参照)。
著作権保護されている作品は、許諾なしに投稿しないでください!
編集を中止
編集の仕方
(新しいウィンドウで開きます)
案内メニュー
個人用ツール
ログインしていません
トーク
投稿記録
アカウント作成
ログイン
名前空間
ページ
議論
日本語
表示
閲覧
編集
履歴表示
その他
検索
案内
メインページ
最近の更新
おまかせ表示
MediaWikiについてのヘルプ
ツール
リンク元
関連ページの更新状況
特別ページ
ページ情報