Aditya L1 Mission: Surya Ka Deep Adhyayan Aur Antariksh Mausam Ki Suraksha | Full Jankari In Hindi

Aditya L1 ek prathamik kakshik Bharatiya surya mission hai jo Suraj ko adhyayan karne ke liye antariksh sthal par sthapit hoga. Vaayumandal aur Bhumisystem ke Suraj-Bhumi L1 Lagrangian bindu ke aas-paas ek halo orbit mein rakha jaane ka iraada hai, jo lagbhag 15 lakh km doori par hoga. L1 bindu ke aas-paas ek halo orbit mein sthit ek upagrah ka mahatvapoorn labh yeh hai ki vah Suraj ko bina kisi avritti/grahan ke lagatar dekhega. Yeh mahatvapoorn labh pradaan karega ki surya gatividhiyon ko lagatar dekhne ka adhik labh hoga.

Yantra saat payloads carry karega jisse prakashkosh, rangakosh aur surya ke sabse bhaari parat (corona) ka adhyayan electromagnetic aur khanij tarkik pakshakar ko upayog karke kiya jaayega. L1 ka vishesh drishtikon istemal karke, char payloads seedhe Suraj ko dekhenge aur shesh teen payloads L1 Lagrange bindu par khanij aur kshetron ke adhyayan ko anukoolit karenge.

Aditya L1 payloads ki samagri ki ummid hai ki yeh mukhya jaankari pradaan karenge jisse coronal heating, Coronal Mass Ejection, pehle-sele aur ukhad gatividhiyon ke samasyaon ko samajhne mein madad milegi, saath hi antariksh aavaas mein kshetron aur khanijon ka prachar ka adhyayan, interplanetary madhyam mein khanijon aur kshetron ke prasaran ki adhyayan, aadi ka adhyayan kiya jaa sakega.”

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Lagrange Bindu

Do-body gurutvakarshan pranali ke liye, Lagrange Bindu woh jagah hote hain jaha antariksh mein par agar ek chhota vastu rakha jaaye toh woh wahan rukne ki pravritti rakhta hai. Aise jagah, jaise ki Suraj aur Prithvi ke liye do-sharir pranali mein, yaaniki Suraj aur Prithvi, upagrah dwara kam jalavayu khapat ke saath in asthano par bane rehne ke liye istemal kiye ja sakte hain.

Technically, Lagrange Bindu par, do bade sharir ki gurutvakarshan akarshan shakti ek chhote vastu ke saath unke saath gati karne ke liye avashyak kendripetal bal ke barabar hoti hai. Do-sharir gurutvakarshan pranali ke liye, kul milake paanch Lagrange Bindu hote hain, jinka naam hai L1, L2, L3, L4, aur L5. Lagrange Bindu L1 Suraj-Prithvi rekha ke beech sthit hai. L1 ki doori Prithvi se lagbhag Prithvi-Suraj doori ka 1% hai.

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Aditya L1 ki Yatra Ki Yojna

Aditya L1 mission ko ISRO ke PSLV XL rocket se Satish Dhawan Space Centre SHAR (SDSC-SHAR), Sriharikota se launch kiya jayega. Shuruwat mein, upagrah ko Ek Low Earth Orbit mein rakha jayega. Uske baad, orbit ko adhik akriti wala banaya jayega aur phir upagrah ko onboard propulsion ka istemal karke Lagrange point (L1) ki or launch kiya jayega.

Jab upagrah L1 ki or yatra karega, tab woh Prithvi ke gurutvakarshan Sphere of Influence (SOI) se bahar niklega. SOI se bahar nikalne ke baad, yatra ka phase shuru hoga aur phir upagrah ko L1 ke aas-paas ek bada halo orbit mein praveshit kiya jayega. Puri yatra ka samay, launch se L1 tak, lagbhag char mahine ka hoga Aditya L1 ke liye.

Aditya L1 ki Visheshta

Aditya L1 mission ka ek visheshta hai ki yeh pahli baar hoga jab hum surya ki nikat ultraviolet kshetra mein ek vistarit chitra dekh sakenge.

Iske alawa, yeh mission surya ke chakkar ke paas, lagbhag surya ke 1.05 solar radius ke nazdik, CME dynamics ko dekhega. Isse hame CME ki gati ke bare mein jankari milegi, jo hamesha se niyamit roop se dekhi nahi jaati.

Is upagrah mein onboard intelligence bhi hogi, jo CMEs aur surya ke tej sitkaron ko pehchanne mein madad karegi. Isse humare observations aur data volume ko behtar bana sakenge.

Aur akhiri visheshta mein, yeh mission surya ke vayu me hone wale disha aur urja anisotropy ko bhi dekhega, kai dishaon se observations karke.

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Vigyanik Lakshya:

Aditya L1 mission ke pramukh vigyanik lakshya hain:

1. Suraj ke upari vatavaran (chromosphere aur corona) ki gatividhiyon ka adhyayan karna.
2. Chromospheric aur coronal garami, adhansh ionized plasma ki bhautik vigyan, coronal mass ejections aur flares ki shuruaat ka adhyayan karna.
3. Suraj se aane wale khanij aur plasma paristhiti ko in-situ dekhkar, Suraj se aane wale khanij ki gatividhiyon ka adhyayan karne ke liye data pradan karna.
4. Suraj ki corona aur uski garami mechanism ki bhautik vigyan.
5. Coronal aur coronal loops plasma ki janch: Tapmaan, gati aur ghanatv.
6. CMEs ki vikas, gatividhi, aur mool.
7. Pahuchte surya ke vibhinn shreniyon (chromosphere, base, aur vistarit corona) mein hone wale prakriyaon ka pata lagana jo ant mein surya ke eruptive ghatnayein utpann karti hain.
8. Suraj ki corona mein chumbak kshetra ki topology aur chumbak kshetra ki measurements.
9. Antariksh mausam ke liye drayvar (mool, mishran aur surya vayu ki gatividhiyon ki utpatti aur gatividhiyon).

Payloads aur unke pramukh vaigyanik anusandhan ki kshamata ke saath.

Remote Sensing Payloads:

1. Visible Emission Line Coronagraph (VELC) – Corona/Chhaya aur Spectroscopy ke liye
2. Solar Ultraviolet Imaging Telescope (SUIT) – Prakashkosh aur Chromosphere Imaging – Sankirn aur Vistarit
3. Solar Low Energy X-ray Spectrometer (SoLEXS) – Soft X-ray Spectrometer: Suraj-ek-taara adhyayan
4. High Energy L1 Orbiting X-ray Spectrometer (HEL1OS) – Hard X-ray Spectrometer: Suraj-ek-taara adhyayan

In-situ Payloads:

5. Aditya Solar wind Particle Experiment (ASPEX) – Surya vayu/Khanij Analyzer Protons aur Bhari Ions ke sath dishaon ke saath
6. Aditya (PAPA) ke liye Plasma Analyzer Package – Surya vayu/Khanij Analyzer Electrons aur Bhari Ions ke sath dishaon ke saath
7. Advanced Tri-axial High Resolution Digital Magnetometers – In-situ Chumbak Kshetra (Bx, By aur Bz).

All Aditya L1 Payloads Images

Suraj ( The Sun )

Hamara Suraj hamare paas ka sabse nikat sitara hai aur surya mandal ka sabse bada vastu hai. Suraj ki anumanit umra lagbhag 4.5 arab varsh hai. Yeh ek garam chamakta hua hydrogen aur helium gas ka gola hai. Prithvi se surya tak ki doori lagbhag 150 arab kilometer hai, aur yeh hamare surya mandal ke liye urja ka srot hai. Suraj ki gurutvakarshan sabhi surya mandal ke vastuon ko ek saath rakhta hai.

Suraj ke madhya bhag ko ‘core’ ke roop mein jana jata hai, jahan par temperature 15 arab degree Celsius tak pahunch sakta hai. Is temperature par, ek prakriya hoti hai jo ‘nuclear fusion’ ke naam se jaani jaati hai aur jo suraj ko shakti pradan karti hai. Suraj ki dikhne wali surface ko ‘photosphere’ ke roop mein jaana jaata hai, aur yeh relatively thandi hoti hai aur uska temperature lagbhag 5,500°C hota hai.

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Suraj Ka Adhyayan Kyun Karein? (WHY STUDY SUN?)

Suraj hamare Saurmandal ka sabse pass ka tara hai aur isliye hum ise anya taron ke tulnatmak roop mein adhik vistar se adhyayan kar sakte hain. Suraj ka adhyayan karke hum apni Milkyway Galaxy mein maujud taron ke baare mein aur vibhinn anya galakshiyon mein maujud taron ke baare mein adhik jaan sakte hain.

Suraj ek atyant gatividhiyon wala tara hai jo hamare dekhe jaane se kahin adhik faila hua hai. Isme kai prakar ke ghatnayein hoti hain aur surya mandal mein bada maatra mein urja chhodta hai. Agar aise prabhal surya ghatnayein prithvi ki or ho, to yeh paas ke antariksh vaatavaran mein vibhinn prakar ke pareshani utpann kar sakti hain.

Vibhinn upagrahon aur sanchar pranaliyon ko aisi ulajhanon ka saamna karna pad sakta hai, isliye aise ghatnaon ki agahin hone ki mahatvapurna baat hai taki pehle se sudharatmak kadam uthaye ja sakein. Iske alawa, agar ek Grah seedhe aisi prabhal ghatnayein se sampark mein aata hai, to uski jindagi khatre mein ho sakti hai.

Suraj par vibhinn ushma aur chumbak ghatnayein atyant prakritik prakriti ki hoti hain. Isliye, suraj bhi un prakriyao ka achha prakritik prayogshala pradan karta hai jinhe seedhe lab mein adhyayan nahi kiya ja sakta.

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Antariksh Mausam ( THE SPACE WEATHER )

Suraj lagatar prithvi par radiations, garami , Particlesl aur chumbak kshetron ka ek sthir pravah bhejta rahta hai. Suraj se aane wale particles ka sthir pravah surya vayu ke roop mein jaana jaata hai aur adhikansh roop se uncha oorja wale protons se mila hota hai. Surya vayu surya mandal ke adhikansh vyapar ko bhar deta hai. Sath hi surya vayu, surya chumbak kshetra bhi surya mandal ko bhar deta hai.

Surya vayu aur anya prabhal/ukhad prabhal surya ghatnayein, jaise ki Coronal Mass Ejection (CME), surya mandal ki prakriti par asar dalte hain. Aisi ghatnayein hone par nikat sthal par planet ke chumbak kshetra aur charge kankal vatavaran ki prakriti badal jaati hai. Prithvi ke case mein, Prithvi ke chumbak kshetra aur CME ke dwara liye gaye chumbak kshetra ke saath ki gayi gatividhi ek chumbak vilakshanata ko prabhavit kar sakti hai. Aisi ghatnayein antariksh sampadaon ke prabhav ko bhi prabhavit kar sakti hain.

Antariksh mausam se matlab hai ki prithvi aur anya grahon ke aas-paas antariksh mein hone wali paristhitiyon mein parivartan. Ham antariksh mein adhik takneek ka istemal karte hain, kyun ki antariksh mausam ko samajhna bahut mahatvapurna hai. Iske alawa, prithvi ke nikat antariksh mausam ko samajhna, anya grahon ke antariksh mausam ke vyavhaar par bhi prakash dalta hai.

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Kyun Karein Suraj Ka Adhyayan Antariksh Se? (WHY STUDY SUN
FROM SPACE?)

Suraj prakriti ke vibhinn tarango mein roshni ko nikalta hai, saath hi saath vibhinn urja se bharpur Particles aur chumbak Tarang bhi nikalta hai. Prithvi ki vaayumandal aur uski chumbak kshetra suraksha kavach ke roop mein kaam karte hain aur kai hanikarak tarango ki roshni, Particles ko rok dete hain. Kyunki vibhinn roshniyan Prithvi ke surface tak nahi pahunchti, isliye Prithvi se aise radiation ko detect karne ke liye upkaran upyogee nahi hote aur surya ke adhyayan jo in radiations par aadharit hain, ve nahi kiye ja sakte hain.

Haalaanki, aise adhyayan ko prithvi ke vaayumandal ke bahar se, yaani ki antariksh se observations karke kiya ja sakta hai. Usi tarah se, samajhne ke liye ki surya vayu ke kankal aur chumbak kshetra suraj se kaise antariksh mein yatra karte hain, vyakti ko prithvi ke chumbak kshetra ke prabhav se door ek sthal se measurements karne ki aavashyakta hoti hai.

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Kya Aditya L1 Suraj Ka Pura Adhyayan Karne Ke Liye Ek Pura Mission Hai? (IS ADITYA L1 A COMPLETE MISSION TO STUDY THE SUN?)

Pratyaksh uttar ‘NA’ hai, jo Aditya L1 ke liye hi nahi, balki aam taur par kisi bhi antariksh mission ke liye sach hai. Iska karan yeh hai ki vaigyanik payloads ko antariksh mein le jaane vale upagrah ke simit maas, shakti aur sthan ki karan se, sirf simit sankhya mein upkaranon ka saath diya ja sakta hai. Aditya L1 ke case mein, sabhi measurements Lagrange bindu L1 se ki jayengi. Ek udaharan ke roop mein, suraj ke vibhinn ghatnayein bahut dishaon mein hoti hain, isliye pradhwamsa/ukhad prabhal ghatnayein ki urja ke dishaik prasaran ko Aditya L1 ke saath hi adhyayan kar pana sambhav nahi hoga.

Ek aur Lagrange bindu L5 ke roop mein ek achha vantage point hai Prithvi ki or ki CME ghatnaon ka adhyayan karne aur antariksh mausam ka moolyaankan karne ke liye. Iske alawa, suraj ke dhruvi kshetra ko achhe se adhyayan nahi kiya gaya hai kyonki is tarah ke adhyayan ke liye upagrah ke mandal prapti ke takneekanshil samasyaon ka samna karna padta hai. Suraj ke dhruvi gatividhiyan aur chumbak kshetra surya chakron ko nikalne mein mahatvapurna bhumika nibhane mein maana jaata hai. Aur bhi to, surya ki vibhinn tarango ki polarisation measurements alag-alag prakashkoshon mein hone wale vibhinn prakriyao ko samajhne ke liye aavashyak hain jo suraj ke aspaas aur andar ghatit hote hain.

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Aditya L1 Surya Mission Ki Top Highlights

1. Antariksh Mein Suraj Ka Adhyayan: Aditya L1 ek prathamik kakshik Bharatiya surya mission hai jo Suraj ko adhyayan karne ke liye antariksh sthal par sthapit hoga. Isse Suraj ke gatividhiyon ka adhyayan kiya jayega.
2. Lagrange Bindu L1: Upagrah ko Lagrange Bindu L1 par sthapit kiya jayega, jo Suraj-Bhumi L1 Lagrangian bindu ke aas-paas ek halo orbit mein sthit hai. Isse Suraj ko lagatar dekhne ka labh milta hai.
3. Saat Payloads: Yantra saat payloads carry karega jinse prakashkosh, rangakosh, aur surya ke sabse bhaari parat (corona) ka adhyayan kiya jayega. Isse surya ke gatividhiyon ko samajhne mein madad milegi.
4. Vigyanik Lakshya: Aditya L1 mission ke vigyanik lakshya mein surya ke upari vatavaran, garami, aur chumbak kshetron ka adhyayan shamil hai. Yeh ghatnayein jaise coronal heating aur Coronal Mass Ejection ko samajhne mein madad karega.
5. Yatra Ki Yojna: Upagrah PSLV XL rocket se launch kiya jayega aur L1 tak pahunchne ke liye char mahine ki yatra ki jayegi.
6. Advanced Instruments: Mission mein visible emission line coronagraph, solar ultraviolet imaging telescope, solar low energy X-ray spectrometer, aur high energy L1 orbiting X-ray spectrometer jaise instruments honge.
7. In-situ Measurements: Aditya L1 upagrah surya vayu aur khanijon ke paristhiti ko in-situ dekhega, jisse suraj se aane wale khanijon ke gatividhiyon ka adhyayan kiya jayega.
8. Antariksh Mausam: Suraj ke gatividhiyon ke adhyayan se antariksh mausam ko samajhne mein madad milegi, jisse upagrahon aur sanchar pranaliyon ke liye suraksha upayog hoga.
9. Space Weather Monitoring: Suraj se aane wale radiations aur gatividhiyon ka nigrani karna antariksh mausam ki samajh mei madad karega aur upagrahon ki suraksha ko sudharne mei sahayak hoga.
10. Surya Ka Adhyayan Antariksh Se: Antariksh se suraj ka adhyayan karke, hamari samajh surya mandal ke vibhinn ghatnaon aur surya vayu ke prabhav ko sudharne mei madadgar hai.

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Aditya L1 Surya Mission Ki Mahatvapurna Visheshtaayein :

11. Ultraviolet Kshetra Ka Adhyayan: Aditya L1 mission pahli baar surya ki nikat ultraviolet kshetra mein ek vistarit chitra dekhega. Isse hume surya ke is mahatvapurna kshetra ke ghatnayein aur prakriti ko samajhne mein madad milegi.
12. CME Dynamics Ka Adhyayan: Mission CME dynamics ko vistrit roop se dekhega aur hume coronal mass ejections ki gati aur prabhav ko samajhne mein madad milegi. Isse antariksh vaatavaran mein hone wale pareshaniyon ka pata lagane mei bhi sahayak hoga.
13. Onboard Intelligence: Upagrah mein onboard intelligence hogi jo CMEs aur surya ke tej sitkaron ko pehchanne mein aur samajhne mein madad karegi. Isse humare observations aur data volume ko behtar bana sakega.
14. Surya Ki Garami Mechanism Ka Adhyayan: Aditya L1 mission surya ki garami mechanism ka bhi bhautik vigyan karega. Isse hume surya ke mahatvapurna garami process ko samajhne mein sahayak hoga.
15. Surya Chakron Ka Adhyayan: Mission surya ke dhruvi kshetra ko adhyayan karega aur chakron ki vyavastha aur gatividhiyon ko samajhne mei madad karega.
16. Polarisation Measurements: Suraj ke vibhinn tarango ki polarisation measurements mission ke moolyankan ko aur adhik vistrit banayenge aur suraj ke vibhinn prakriyao ko samajhne mei sahayak honge.
17. Surya Vayu Ka Adhyayan: Aditya L1 mission surya vayu aur uske gatividhiyon ka adhyayan karega, jisse hum surya se aane wale protons aur bhari ions ke saath dishaon ke saath prabhav ko samajh sakenge.
18. Antariksh Sampadaon Ke Prabhav Ka Pata Lagana: Mission antariksh mausam ke prabhav ko bhi dekhega, jisse antariksh sampadaon ke prabhav ko samajhne mei madadgar hoga.
19. Remote Sensing Payloads: Visible emission line coronagraph, solar ultraviolet imaging telescope, solar low energy X-ray spectrometer, aur high energy L1 orbiting X-ray spectrometer jaise remote sensing payloads upagrah par honge.
20. In-situ Chumbak Kshetra: Upagrah par advanced tri-axial high-resolution digital magnetometers honge jo in-situ chumbak kshetra measurements karenge.

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Aditya L1 Surya Mission ke Pros

1. Surya Ka Gahra Adhyayan: Aditya L1 mission suraj ko antariksh se gahri roshni mein adhyayan karne ka mauka pradan karega, jisse hum suraj ke gatividhiyon, urja prasaran aur chumbak tarangon ko samajh sakte hain.
2. Lagrange Bindu L1: Upagrah ko Lagrange Bindu L1 par sthapit karke suraj ko bina kisi avritti/grahan ke lagatar dekhne ka labh milega, jisse suraj ke gatividhiyon ka adhyayan kiya ja sakega.
3. Vigyanik Lakshya: Mission ke vigyanik lakshya, jaise coronal heating, Coronal Mass Ejection, aur surya ke gatividhiyon ko samajhne mein madad karenge, jisse antariksh vaatavaran mein hone wale pareshaniyon ka pata lagaya ja sakega.
4. Antariksh Mausam Ka Moolyaankan: Suraj se aane wale radiations aur gatividhiyon ka nigrani karna antariksh mausam ki samajh mei madad karega, jisse upagrahon aur sanchar pranaliyon ke liye suraksha upayog hoga.
5. Surya Ka Adhyayan Antariksh Se: Antariksh se suraj ka adhyayan karke, humari samajh surya mandal ke vibhinn ghatnaon aur surya vayu ke prabhav ko sudharne mei madadgar hai.
6. Advanced Instruments: Mission mein upkaran jaise visible emission line coronagraph, solar ultraviolet imaging telescope, solar low energy X-ray spectrometer, aur high energy L1 orbiting X-ray spectrometer honge, jo suraj ke gatividhiyon ko vistrit roop se dekhne mein sahayak honge.
7. In-situ Measurements: Aditya L1 upagrah surya vayu aur khanijon ke paristhiti ko in-situ dekhega, jisse suraj se aane wale khanijon ke gatividhiyon ka adhyayan kiya jayega.

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Aditya L1 Surya Mission ke Cons

1. Limited Payloads: Antariksh mission ke liye simit maas, shakti, aur sthan ki karan se, mission ke upagrah par simit sankhya mein upkaran hi saath diye ja sakte hain, jisse kuch ghatnayein ya measurements miss ho sakte hain.
2. Surya Ke Vibhinn Ghatnayein: Suraj ke vibhinn ghatnayein bahut dishaon mein hoti hain, jisse pradhwamsa/ukhad prabhal ghatnayein ki urja ke dishaik prasaran ko Aditya L1 ke saath hi adhyayan kar pana sambhav nahi hoga.
3. Surya Ke Dhruvi Kshetra Ka Adhyayan: Mission surya ke dhruvi kshetra ko adhyayan nahi kar sakta hai, jo suraj ke mahatvapurna gatividhiyon ka ek mahatvapurna hissa hai.
4. Polarisation Measurements Ki Kami: Suraj ke vibhinn tarango ki polarisation measurements ki kami se kuch prakriyao ko samajhne mein sankoch ho sakta hai.
5. Space Weather Monitoring: Suraj se aane wale radiations aur gatividhiyon ka nigrani karna antariksh mausam ki samajh mei madad karta hai, lekin mission se aane wale data ke samay par sahi upayog ke liye ek pranali banani hogi.
6. Mission Ka Samay: Aditya L1 mission ki yatra L1 tak char mahine tak ka samay lagega, jo mission ko lamba bana sakta hai.
7. Cost and Resources: Antariksh mission ke liye bade kharche aur sansadhan ki aavashyakta hoti hai, jo ki sarkar aur ISRO ke liye ek maamuli chunauti ho sakti hai.
8. Mission Ke Baadke Upagrah Ka Prabandhan: Mission ke baad upagrah ka prabandhan aur suraksha ek mahatvapurna uttaradayitva hai, aur iska vyavasthit roop se kiya jana chahiye.

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FAQs

1. Aditya L1 mission kya hai?

Aditya L1 mission ek Bharatiya antariksh mission hai jo Suraj ko adhyayan karne ke liye sthapit kiya gaya hai. Is mission mein Suraj ke gatividhiyon aur antariksh mausam ke prabhav ko samajhne ke liye upagrah L1 Lagrange bindu par sthapit hoga.

2. Lagrange bindu kya hota hai?

Lagrange bindu ek aisa sthal hai antariksh mein jahan par agar ek chhota vastu rakha jaaye toh woh wahan rukne ki pravritti rakhta hai. Aditya L1 mission Lagrange bindu L1 par sthapit hoga, jo Suraj-Bhumi L1 Lagrangian bindu ke aas-paas ek halo orbit mein sthit hai.

3. Aditya L1 mission ke kitne payloads honge?

Aditya L1 mission mein saat payloads honge. In payloads mein prakashkosh, rangakosh, aur surya ke sabse bhaari parat (corona) ka adhyayan kiya jayega, aur surya ke gatividhiyon ko samajhne mein madad milegi.

4. Aditya L1 mission ke vigyanik lakshya kya hain?

Aditya L1 mission ke vigyanik lakshya mein suraj ke upari vatavaran, garami, aur chumbak kshetron ka adhyayan shamil hai. Isse coronal heating, Coronal Mass Ejection, aur antariksh mausam ko samajhne mein madad milegi.

5. Aditya L1 upagrah ki yatra ki yojna kya hai?

Aditya L1 upagrah ko PSLV XL rocket se launch kiya jayega. Shuruwat mein, upagrah Ek Low Earth Orbit mein rakha jayega, uske baad L1 ki or yatra karega aur ek bada halo orbit mein sthapit kiya jayega. Puri yatra ka samay lagbhag char mahine ka hoga.

6. Aditya L1 mission ke kuch visheshtaayein kya hain?

Aditya L1 mission ki kuch visheshtaayein hai, jaise surya ki nikat ultraviolet kshetra mein ek vistarit chitra dekhna, CME dynamics ka adhyayan, onboard intelligence, aur surya chakron ka adhyayan.

7. Suraj ka adhyayan antariksh se kyun karna zaroori hai?

Suraj ka adhyayan antariksh se zaroori hai kyun ki Suraj prakriti ke vibhinn tarango mein roshni aur urja ko nikalta hai, aur iska adhyayan prithvi ke chumbak kshetra aur antariksh mausam ke liye mahatvapurna hai.

8. Kya Aditya L1 mission suraj ka poora adhyayan karne ke liye pura mission hai?

Nahi, Aditya L1 mission pura suraj ka adhyayan nahi kar sakta hai kyun ki suraj ke gatividhiyan vibhinn dishaon mein hoti hain. Is mission mein Lagrange bindu L1 par adhyayan kiya jayega, lekin aur adhyayan ke liye dusre sthal bhi avashyak hain, jaise Lagrange bindu L5.

9. Aditya L1 Surya Mission ki kya top highlights hain?

Aditya L1 Surya Mission ki top highlights mein include hain antariksh mein suraj ka adhyayan, Lagrange bindu L1 ka upayog, saat payloads, vigyanik lakshya, yatra ki yojna, advanced instruments, in-situ measurements, antariksh mausam ka moolyaankan, aur suraj se aane wale radiations aur gatividhiyon ka nigrani karna.

10. Aditya L1 Surya Mission ka adhyayan kis tarah se hume fayda pahuncha sakta hai?

Aditya L1 Surya Mission ka adhyayan hume suraj ke gatividhiyon, antariksh mausam, aur surya se aane wale radiations ke prabhav ko samajhne mein madad pahuncha sakta hai. Isse upagrahon ki suraksha aur antariksh vaatavaran ki samajh mei sudhar kiya ja sakta hai.