What is the translation of " SUNČEV VJETAR " in English?

• solar wind

Examples of using Sunčev vjetar in Croatian and their translations into English

Sunčev vjetar teče od lijeva na desno.
The solar wind flows from left to right.

To znači da Sunce izgubi oko 0.01% svoje ukupne mase kroz Sunčev vjetar.
Only about 0.01% of the Sun's total mass has been lost through the solar wind.

Sunčev vjetar je preslab To je neuravnoteženo.
It's unbalanced. The solar wind is too weak.

Godine 1959. je sovjetski satelit Luna 1 prvi uočio Sunčev vjetar i mjerio njegovu jačinu.
In January 1959, the Soviet satellite Luna 1 first directly observed the solar wind and measured its strength.

Sunčev vjetar je brzo otjecanje vruće plazme sa Sunca u svim smjerovima.
The solar wind is a fast outflow of hot plasma from the sun in all directions.

Ionosfere magnetski slabih planeta Venere i Marsa, djelomično odbijaju Sunčev vjetar.
The ionospheres of weakly magnetized planets such as Venus and Mars set up currents that partially deflect the solar wind flow around the planet.

Time je objasnio da se Sunčev vjetar sastoji od negativnih elektrona i pozitivnih iona.
The Solar Wind consists of both negative electrons and positive ions.

Budući da Sunce rotira oko svoje osi za otprilike 27 dana, magnetsko polje koje prenosi Sunčev vjetar je zavijeno u spiralu.
As the Sun rotates once in about 27 days, the magnetic field transported by the solar wind gets wrapped into a spiral.

Sunčev vjetar se može podijeliti na spori Sunčev vjetar i brzi Sunčev vjetar.
The solar wind is divided into the slow solar wind and the fast solar wind.

Budući da Sunce rotira oko svoje osi za otprilike 27 dana, magnetsko polje koje prenosi Sunčev vjetar je zavijeno u spiralu.
Because the Sun rotates once approximately every 25 days, the magnetic field transported by the solar wind gets wrapped into a spiral.

Brzi Sunčev vjetar ima brzinu oko 750 km/s, nižu temperaturu oko 8×105 K i ima sastav kao fotosfera.
The fast solar wind has a typical velocity of 750 km/s, a temperature of 8×105 K and nearly matches the photosphere's.

Znanstvenici nagađaju da je nedostatak magnetskog štita pomogao u tome da sunčev vjetar tijekom nekoliko milijardi godina otpuše većinu atmosfere Marsa.
Scientists speculate that the lack of magnetic shielding helped the solar wind blow away much of Mars's atmosphere over the course of several billion years.

I sunčev vjetar, bilo bi prihvatljivo. još nešto da možeš ubaciti u kutiju Nakon što dobiješ cijev jezgre.
Anything else that you can throw into the box would be acceptable. After you have got the core tubes and the solar wind.

Magnetosfera se stvara kada struja električki nabijenih čestica, kao što je sunčev vjetar, međusobno djeluju i skreću, uslijed djelovanja Zemljinog magnetskog polja.
A magnetosphere is formed when a stream of charged particles, such as the solar wind, interacts with and is deflected by the magnetic field of a planet or similar body.

I sunčev vjetar, bilo bi prihvatljivo. još nešto da možeš ubaciti u kutiju Nakon što dobiješ cijev jezgre.
And the solar wind, anything else that you can throw into the box would be acceptable. After you have got the core tubes.

Jedna mogućnost je da elektrodinamični efekti povezani sa razbijanjem materijala u blizini površine mogu dovesti do naboja plinova, kao i sunčev vjetar.
One possibility is that electrodynamic effects related to the fracturing of near-surface materials could charge any gases that might be present, such as implanted solar wind or radiogenic daughter products.

Sunčev vjetar stvara heliosferu, ogroman prostor međuplanetarne tvari, koja okružuje Sunčev sustav.
The solar wind creates the Heliosphere, a vast bubble in the interstellar medium surrounding the Solar System.

Na koju se god planetu spuste, ženka ispusti feromon da je mužjaci mogu pratiti, nađu je, razmnože se itd. Pa možda se kreću svemirom koristeći sunčev vjetar, kao… spore.
Ind it, breed, et cetera. Well, maybe they like drift through space on… on solar winds, like spores, and… whatever planet they land on first, the female leaves a pheromone trail for the males to follow it.

Poznato je da brzi Sunčev vjetar putuje duž silnica otvorenog magnetskog polja, koje prolaze kroz koronalne šupljine.
The escaping solar wind is known to travel along open magnetic field lines that pass through the coronal hole area.

Na koju se god planetu spuste, ženka ispusti feromon da je mužjaci mogu pratiti, nađu je, razmnože se itd. Pa možda se kreću svemirom koristeći sunčev vjetar, kao… spore.
Well, maybe they like drift through space on… on solar winds, like spores, ind it, breed, et cetera. the female leaves a pheromone trail for the males to follow it, and… whatever planet they land on first.

Brzi Sunčev vjetar polazi iz koronalnih šupljina, koje su područja otvorenog magnetskog polja i najviše ih ima na polovima.
The fast solar wind originates from coronal holes, which are funnel-like regions of open field lines in the Sun's magnetic field.

S druge strane, brzi Sunčev vjetar ima brzinu oko 750 km/s, nižu temperaturu oko 8×105 K i ima sastav kao fotosfera.
By contrast, the fast solar wind has a typical velocity of 750 km/s, a temperature of 8×105 K and it nearly matches the composition of the Sun's photosphere.

Spori Sunčev vjetar ima brzinu od oko 400 km/s, temperaturu od oko 1.4- 1.6×106 K i sastav koji je sličan koroni.
The slow solar wind has a velocity of about 400 km/s, a temperature of 1.4- 1.6×106 K and a composition that is a close match to the corona.

Djelujući kao prepreka za ovaj sunčev vjetar, misli se da se spriječi da ove čestice prenesu dovoljno svoje energije na molekule gasa-plina u atmosferi da bi isti pobjegli iz Zemljinog gravitacionog polja.
By acting as a barrier to this solar wind, it is also thought to prevent these particles transferring enough of their energy to gas molecules in the atmosphere for these molecules to escape the Earth's gravitational pull.

Na primjer, Sunčev vjetar djeluje na Zemljinu magnetosferu, stvarajući polarnu svjetlost i Birkelandovu struju.
For example, in the solar wind they interact with the Earth's magnetosphere giving rise to Birkeland currents and the aurora.

Spori Sunčev vjetar ima brzinu oko 400 km/s, temperaturu oko 1, 4- 1, 6 ∙ 106 K i sastav koji je sličan koroni.
The slow solar wind is observed to have a velocity of 300-500 km/s, a temperature of 1.4-1.6×106 K and a composition that is a close match to the corona.

Za vrijeme širenja, ono međusobno djeluje sa Sunčevim vjetrom i međuplanetarnim magnetskim poljem.
During their propagation, CMEs interact with the solar wind and the interplanetary magnetic field IMF.

Vanjski dijelovi korone stalno gube masu u obliku Sunčevog vjetra.
Fortunately, the Sun continuously sheds some of its outer layer in the form of solar wind.

Letna platforma Venere 11 je nosila detektore Sunčeva vjetra, ionosferske elektronske instrumente i dva detektora naleta gama-čestica- sovjetski KONUS i francuski SIGNE 2.
Venera 11 flight platform carried solar wind detectors, ionosphere electron instruments and two gamma ray burst detectors- the Soviet-built KONUS and the French-built SIGNE 2.

Zemlja je dobro zaštićena od Sunčevog vjetra vlastitim magnetskim poljem, koji odbija većinu električki nabijenih čestica.
Earth itself is largely protected from the solar wind by its magnetic field, which deflects most of the charged particles; however some of the charged particles are trapped in the Van Allen radiation belt.