Indian Missiles and Munitions Discussion

I was going through some old docs and I found this :
View attachment 14396

This was put out on 7th March of 2018 by the then RM Mrs. N. Sitharaman. Most of the projects here seem to be on track. Guided Pinaka was tested in December. MRSAM, LRSAM acquisition is on track. DRDO's AIP has been undergoing testing for a long time now. NASM-SR is supposed to be completed by the end of 2021. Interestingly SMART was supposed to end before NASM-SR, but we've seen nothing of it so far. SLCM is an off-shoot of the Nirbhay missile. Details of Rudra M-II/M-II are not public.

What is the difference between Mission Mode Projects and Technology Demonstration Projects ??
 
What is the difference between Mission Mode Projects and Technology Demonstration Projects ??
Welcome back..

I have no idea. But I suppose the only visible difference on the surface is that the mission mode projects are assured to receive purchase orders or have already received orders already. TD projects first need to prove their tech then prospects of acquisition open up.
 
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Re-Engineered Meteor BVRAAM On The Works For IAF

Saturday, February 29, 2020

Meteor BVRAAM Cutaway.jpg


If any new-generation BVRAAM is to become a ‘game-changer’, then it has to have vastly improved kinematic capability compared with that of existing BVRAAMs. This requires substantial increases in two key parameters: ‘F-Pole’, i.e. the distance between the BVRAAM-launching MRCA and its target when the BVRAAM hits; and a ‘no-escape zone’, the range within which the BVRAAM can be fired and the target, no matter how it manoeuvres, cannot escape. When an existing BVRAAM the like AIM-120D AMRAAM, MICA or R-77/RVV-AE is fired at a target, it delivers the same amount of thrust over a certain period regardless of the tactical scenario. If the target can be reached without the rocket motor burning out, or shortly after it does so, the BVRAAM will have a high-energy state during its terminal attack phase. This will allow it to manoeuvre very hard, easily countering a targeted combat aircraft trying to evade the incoming BVRAAM. If the target is farther away, the BVRAAM will usually climb to a high altitude while its rocket motor is burning and then coast on its built-up energy with gravity on its side until it reaches the terminal phase of its flight (its final attack run. If the target is not too far away, and the BVRAAM is still above it, it will dive down on the target in an attempt to maximize its ability to make hard manoeuvres. The longer the shot, the less energy the BVRAAM will have for its critical terminal phase of flight.

Astra-1 BVRAAM's Ku-band Seeker.jpg


Whereas the AMRAAM’s rocket motor burns for seconds, then the missile coasts, a Meteor-type BVRAAM is under ramjet thrust for its complete flight. Consequently, the latter’s average velocity is higher and the Meteor arrives with the energy to out-manoeuvre its target. Thus, both the F-Pole and the no-escape zone are increased. Instead of burning off all its fuel right after launch it can throttle its engine back during cruise, thus saving fuel. As it approaches its target it can throttle up, eventually making its terminal attack while at its highest possible energy state, around Mach 4.5, even when fired over long ranges. Not only does this mean the Meteor will have more energy to manoeuvre during the endgame of the engagement, but this capability also drastically increases the size of the no-escape zone. Basically, the Meteor has a far greater ability to chase and catch enemy combat aircraft over long ranges.

Astra-1 BVRAAM's Ku-band Seeker Developed by RCI.jpg


The Meteor’s data-link also has two-way capability, so the pilot could re-target the BVRAAM while it is already on its way. The pilot can also see the Meteor’s fuel-burn rate, kinematic energy and tracking state in real-time. This is essential for making quick decisions as to whether or not to fire another BVRAAM at the target or to run away if it is properly tracking toward the target or has obtained its own lock. The Meteor will be able to get those crucial mid-course guidance updates not just from the MRCA that fired it, but from “third party” sources as well. These can include other MRCAs, airborne early warning & control (AEW & C) platforms, and land and sea-based radar and electronic surveillance systems that provide their own situational awareness data to the missile-firing MRCA via data-link. Thus, with many assets contributing to a common tactical network “picture” via common data-link waveform and language, it provides information that anyone, including the Meteor-armed BVRAAM and the Meteor itself, can exploit.

Stores Management System.jpg


While the above-mentioned reasons are precisely why the Indian Air Force (IAF) has ordered the MBDA-developed Meteor BVRAAMs for its 36 Rafale M-MRCAs, the operational requirement for such ramjet-powered BVRAAMs is for 2,500 units. And there’s another catch: the Meteor BVRAAM should be compatible with the mission avionics of all types of MRCAs that are in service with the IAF. This, in turn, represents a systems integration challenge, but there is a solution, nevertheless. This involves, on one hand the installation of indigenous mission computer, stores management system and pylon interface avionics (all using the MIL-STD-1760 digital databus) on MRCAs like the Tejas Mk.1, Tejas Mk.1A, Super Su-30MKI and MiG-29UPG, while on the other the Meteor’s MBDA-developed Ku-band active seeker and a module of its rear-mounted two-way data-link can be replaced by corresponding India-supplied avionics and sensors that are used by the indigenously-developed Astra-1 BVRAAM. This way, the MMRs of Russia- and Israel-origin can seamlessly be integrated with the Meteor BVRAAM, since India will first have the avionics and sensors integrated with the Israel-origin and Russia-origin MMRs at the Israel-based and Russia-based avionics integration test-rigs and then supply them to MBDA for installation inside the Meteor airframes.

Astra-2 BVRAAM with SFDR-1.jpg

Astra-2 BVRAAM with SFDR-3.jpg

Astra-2 BVRAAM with SFDR-2.jpg


Engineering studies to this effect were jointly undertaken by MBDA and India’s Defence R & D Organisation (DRDO) back in 2016, when the DRDO began its own in-house conceptual studies on develop a solid-fuel ducted rocket (SFDR)-powered BVRAAM. It then emerged that a suitably-modified Meteor BVRAAM containing DRDO-developed avionics was indeed possible to both develop and integrate with the Russia-/Israel-supplied AESA-MMRs, while at the same time not violating the IPRs of the MMR-supplying foreign OEMs. In fact, MBDA is already well into such a re-engineering programme for Japan, with whom the UK first began holding exploratory talks in 2014 on the prospects of a Meteor BVRAAM fitted with an AESA-based Ka-band millimetric frequency seeker that was developed by Mitsubishi Electric Co (MELCO) in the previous decade for the indigenously developed AAM-4B (Type-99) BVRAAM. Later, in January 2017 the Cooperative Research Project on the Feasibility of a Joint New Air-to-Air Missile (JNAAM) commenced. If all goes well, then such a BVRAAM will begin flight-tests in 2023.

AMP.jpg


In India too, R & D work began in 2016 for developing AESA-based X-band and Ku-band active seekers for both the XR-SAM long-range surface-to-air missile and the SFDR-powered Astra-2 BVRAAM, with Hyderabad-based Astra Microwave already having developed two types of such seekers, with work now underway on developing their Ka-band successors that too will be compatible with the Meteor BVRAAM. The Ka-band seeker with an active phased-array antenna (with 20km-range) and a secondary X-band passive channel will replace existing Ku-band seekers (with 6km-range) and provide higher resolution and countermeasures resistance. Such seekers can effortlessly work across multiple frequencies simultaneously, which makes them not only better at finding objects, but are also more difficult to detect. In addition, electronically steered antenna beams also offer other improvements: it is possible to perform an adaptive antenna beam-forming based on antenna sub-group transmit (Tx) and receive (Rx) channels or even adjusting all the single antenna transceiver elements. This put us into a position to use algorithms of super resolution in order to recognise and localise jammer sources while concurrently conducting target acquisition and tracking.

Meteor BVRAAM with MELCO-Developed AESA Seeker.jpg


TRISHUL: Re-Engineered Meteor BVRAAM On The Works For IAF
 
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I was going through some old docs and I found this :
View attachment 14396

This was put out on 7th March of 2018 by the then RM Mrs. N. Sitharaman. Most of the projects here seem to be on track. Guided Pinaka was tested in December. MRSAM, LRSAM acquisition is on track. DRDO's AIP has been undergoing testing for a long time now. NASM-SR is supposed to be completed by the end of 2021. Interestingly SMART was supposed to end before NASM-SR, but we've seen nothing of it so far. SLCM is an off-shoot of the Nirbhay missile. Details of Rudra M-II/M-II are not public.
Stealth wing flying test bed: ghatak?
Says that it's supposed to be finished by April 2020?? Any chance of seeing that fly? That would be a sight to watch!!
 
Stealth wing flying test bed: ghatak?
A miniature version of Ghatak. Powered by the Russian NPO Saturn 36MT engine. The test is to prove the CLAWs of the Ghatak UCAV.
Says that it's supposed to be finished by April 2020?? Any chance of seeing that fly? That would be a sight to watch!!
Unlikely to be made public anytime soon given the secrecy of the project. Would love to be wrong though.
 
Re-Engineered Meteor BVRAAM On The Works For IAF

Saturday, February 29, 2020
View attachment 14463

If any new-generation BVRAAM is to become a ‘game-changer’, then it has to have vastly improved kinematic capability compared with that of existing BVRAAMs. This requires substantial increases in two key parameters: ‘F-Pole’, i.e. the distance between the BVRAAM-launching MRCA and its target when the BVRAAM hits; and a ‘no-escape zone’, the range within which the BVRAAM can be fired and the target, no matter how it manoeuvres, cannot escape. When an existing BVRAAM the like AIM-120D AMRAAM, MICA or R-77/RVV-AE is fired at a target, it delivers the same amount of thrust over a certain period regardless of the tactical scenario. If the target can be reached without the rocket motor burning out, or shortly after it does so, the BVRAAM will have a high-energy state during its terminal attack phase. This will allow it to manoeuvre very hard, easily countering a targeted combat aircraft trying to evade the incoming BVRAAM. If the target is farther away, the BVRAAM will usually climb to a high altitude while its rocket motor is burning and then coast on its built-up energy with gravity on its side until it reaches the terminal phase of its flight (its final attack run. If the target is not too far away, and the BVRAAM is still above it, it will dive down on the target in an attempt to maximize its ability to make hard manoeuvres. The longer the shot, the less energy the BVRAAM will have for its critical terminal phase of flight.

View attachment 14464

Whereas the AMRAAM’s rocket motor burns for seconds, then the missile coasts, a Meteor-type BVRAAM is under ramjet thrust for its complete flight. Consequently, the latter’s average velocity is higher and the Meteor arrives with the energy to out-manoeuvre its target. Thus, both the F-Pole and the no-escape zone are increased. Instead of burning off all its fuel right after launch it can throttle its engine back during cruise, thus saving fuel. As it approaches its target it can throttle up, eventually making its terminal attack while at its highest possible energy state, around Mach 4.5, even when fired over long ranges. Not only does this mean the Meteor will have more energy to manoeuvre during the endgame of the engagement, but this capability also drastically increases the size of the no-escape zone. Basically, the Meteor has a far greater ability to chase and catch enemy combat aircraft over long ranges.

View attachment 14465

The Meteor’s data-link also has two-way capability, so the pilot could re-target the BVRAAM while it is already on its way. The pilot can also see the Meteor’s fuel-burn rate, kinematic energy and tracking state in real-time. This is essential for making quick decisions as to whether or not to fire another BVRAAM at the target or to run away if it is properly tracking toward the target or has obtained its own lock. The Meteor will be able to get those crucial mid-course guidance updates not just from the MRCA that fired it, but from “third party” sources as well. These can include other MRCAs, airborne early warning & control (AEW & C) platforms, and land and sea-based radar and electronic surveillance systems that provide their own situational awareness data to the missile-firing MRCA via data-link. Thus, with many assets contributing to a common tactical network “picture” via common data-link waveform and language, it provides information that anyone, including the Meteor-armed BVRAAM and the Meteor itself, can exploit.

View attachment 14466

While the above-mentioned reasons are precisely why the Indian Air Force (IAF) has ordered the MBDA-developed Meteor BVRAAMs for its 36 Rafale M-MRCAs, the operational requirement for such ramjet-powered BVRAAMs is for 2,500 units. And there’s another catch: the Meteor BVRAAM should be compatible with the mission avionics of all types of MRCAs that are in service with the IAF. This, in turn, represents a systems integration challenge, but there is a solution, nevertheless. This involves, on one hand the installation of indigenous mission computer, stores management system and pylon interface avionics (all using the MIL-STD-1760 digital databus) on MRCAs like the Tejas Mk.1, Tejas Mk.1A, Super Su-30MKI and MiG-29UPG, while on the other the Meteor’s MBDA-developed Ku-band active seeker and a module of its rear-mounted two-way data-link can be replaced by corresponding India-supplied avionics and sensors that are used by the indigenously-developed Astra-1 BVRAAM. This way, the MMRs of Russia- and Israel-origin can seamlessly be integrated with the Meteor BVRAAM, since India will first have the avionics and sensors integrated with the Israel-origin and Russia-origin MMRs at the Israel-based and Russia-based avionics integration test-rigs and then supply them to MBDA for installation inside the Meteor airframes.

View attachment 14467
View attachment 14468
View attachment 14471

Engineering studies to this effect were jointly undertaken by MBDA and India’s Defence R & D Organisation (DRDO) back in 2016, when the DRDO began its own in-house conceptual studies on develop a solid-fuel ducted rocket (SFDR)-powered BVRAAM. It then emerged that a suitably-modified Meteor BVRAAM containing DRDO-developed avionics was indeed possible to both develop and integrate with the Russia-/Israel-supplied AESA-MMRs, while at the same time not violating the IPRs of the MMR-supplying foreign OEMs. In fact, MBDA is already well into such a re-engineering programme for Japan, with whom the UK first began holding exploratory talks in 2014 on the prospects of a Meteor BVRAAM fitted with an AESA-based Ka-band millimetric frequency seeker that was developed by Mitsubishi Electric Co (MELCO) in the previous decade for the indigenously developed AAM-4B (Type-99) BVRAAM. Later, in January 2017 the Cooperative Research Project on the Feasibility of a Joint New Air-to-Air Missile (JNAAM) commenced. If all goes well, then such a BVRAAM will begin flight-tests in 2023.

View attachment 14470

In India too, R & D work began in 2016 for developing AESA-based X-band and Ku-band active seekers for both the XR-SAM long-range surface-to-air missile and the SFDR-powered Astra-2 BVRAAM, with Hyderabad-based Astra Microwave already having developed two types of such seekers, with work now underway on developing their Ka-band successors that too will be compatible with the Meteor BVRAAM. The Ka-band seeker with an active phased-array antenna (with 20km-range) and a secondary X-band passive channel will replace existing Ku-band seekers (with 6km-range) and provide higher resolution and countermeasures resistance. Such seekers can effortlessly work across multiple frequencies simultaneously, which makes them not only better at finding objects, but are also more difficult to detect. In addition, electronically steered antenna beams also offer other improvements: it is possible to perform an adaptive antenna beam-forming based on antenna sub-group transmit (Tx) and receive (Rx) channels or even adjusting all the single antenna transceiver elements. This put us into a position to use algorithms of super resolution in order to recognise and localise jammer sources while concurrently conducting target acquisition and tracking.

View attachment 14469

TRISHUL: Re-Engineered Meteor BVRAAM On The Works For IAF

Some more photos :

Astra-1 SOC FOC gyro :
Astra-1's System-on-Chip for Fibre-Optic Gyro.jpg


Astra-1 Seeker components :
Astra-1 Seeker Components.jpg


RF seekers by DRDO so far :
RF Seekers.jpg
 
How close can we say is the Helina for certification?

Feb-2020

In the last one year we saw multiple success on the missile front. Various trials of Astra, quick reaction surface to air missile (QRSAM ), Nag and Pinaka were successfully completed.

This year the user trials of HELINA missile and man portable anti tank guided missile (MPATGM) will be completed. Development trials of new generation anti radiation missile (NGARM ) will be taken up this year. We are also working on Astra Mk-2 long range air-to-air missile. There are several other missiles that are in the pipeline.

On the weapons front, we have developed the Advanced Towed Artillery Gun System (ATAGS) in collaboration with Tatas and Bharat Forge. This year the system will undergo user trials. We are also developing the Joint Venture Protective Carbine (JVPC) and smart anti-airfield weapon (SAAW) bomb.

I am confident that SAAW will complete its trials this year and enter into production. There are many other weapons also being developed simultaneously.

INTERVIEW | Youngsters can power India into a defence technology leader: Dr Satheesh Reddy
 
😅😅😅😅😅😅😅
You Indians Never fail to amuse me

He's right actually - I don't see how an MKU-made ACH can find its way abroad considering its still in production and no chance for there to be military surplus at this stage.

Plus, that camo on the helmet cover is US M81 Woodland, definitely not Indian PC Disruptive. You can tell by the shape of the black swatches.

M81 Woodland -

%22M81%22_U.S._woodland_camouflage_pattern_swatch.png


Third, MKU helmet covers come with moulded rubber liner on the edge of the helmet as standard, the one in video doesn't have it. It's clearly not Indian camo, so no real reason to think the helmet is genuine MKU either. Looks like a generic ACH with generic woodland cover one can buy on Amazon.

D18f-vFUkAUn9mM

BE218.JPG
 
😅😅😅😅😅😅😅
You Indians Never fail to amuse me
Bhai jaan if you had seen his older videos you would have known by now that he used an American ach and put an Indian flag on it. Also we don't use these helmets because most of our military actually is using model 74 which is worse than this. And there is no chance that some random gora will get hands on the new mku/Tata helmets. He was clickbaiting and abduls like you took his words as gospel.