The conical RV of Agni P is a step up or a generation ahead of what we call BGRV in Indian parlance. Agni-2 was the first Indian ballistic missile to use Ballistic glide reentry vehicle . Here's Agni P RV.
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Here's the Common Hypersonic Glide body of the American LRHW . The RV is made by Dynetics and the boosters are made by LM.
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CHRB is a proper hypersonic glide vehicle. Notice its close resemblance to the Agni P RV. What's different is that the Agni RV doesn't have the fixed delta wings but has smaller clipped movable fins. Instead it has a thicker higher dia blunt nose compared to CHGB. So whatever lift that these deltas generated is compensated by the blunt nose tip which gives the conical RV a higher L to D coefficient compared to the pointed nose of CHGB.
These are the different classes of HGV that have already flight tested or are in developement now.
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That conical body is a Pershing-2 RV. CHRB is closer to delta winged body. Our conical RV has a LD ratio of 3.5+. Its a true blue HGV . Previously we had Shaurya as a quasi ballistic / hypersonic glide vehicle. Before that there was Agni-2 BGRV.
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In one test in 2011, Shaurya flew for 700 kms at just 40 km alt. It cruised at around M7.5. Look at the two radar horizon slant lines in the above pic. Shaurya will be undetectable for most of its trajectory due to its low flight alt. Shaurya is a true blue HGV. We had entered the hypesonics club more than a decade back. Remember this and always feel extra proud for being born here. We are part of an elite grouping and we have already earned a place at the high table.
Now here's the flight profile of CHRB during one of its tests.
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More than 3/4th of the distance was spent gliding . Agni P is distinct here due to the fact that in all probability it has a small solid rocket motor mated to a flex nozzle in the RV which not only allows for complex 3D maneuvering in exo atmosphere in conjunction with the DACS but it also provides a degree of continuous propulsion within atm so as to sustain the flight speeds. Within atm as the heigh decreases ,the air becomes denser and any HGV cruising here rapidly looses speed and energy due to high drag. A sustained motor with a flex nozzle alleviates this problem to a huge extent and allows for high terminal speeds . The fins help in providing aerodynamic control inside atm similar to a MaRV. DACS is also partially effective in the higher parts of atmosphere. All these manuevering both exo and endo atmosphere will help Agni-P RV to hit a frigate class moving warship with single digit CEP.
Agni-P is the basis of the upcoming LRAShM. Only an imaging X band seeker and a radome able to sustain the high Mach nos are needed. A heat shield can also be used which will be jettisoned once within a few hundred kms of the warship. W band seeker has very small ranges and won't be applicable here.