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  • The role of water vapor and cloud feedback on the evolution of the Indian summer monsoon

    over the last 22,000 years

    Chetankumar Jalihal

    Guided by: Prof. J. Srinivasan &Prof. Arindam Chakraborty

    jalihal@iisc.ac.in Indian Institute of Science

    mailto:jalihal@iisc.ac.in

  • Short version

  • OBJECTIVE

    DIFFERENT SENSITIVITY OF

    MONSOON TO INSOLATION

    1

    TraCE21K simulation

    Model: CCSM3, fully coupled ESM, with transient boundary conditions,3.75ᵒ x 3.75ᵒ

    Duration: 22 Kyrs

  • OBJECTIVE

    OBJECTIVE

    Identify the feedbacks.

    Quantify the role of forcings and feedbacks.

    2

  • 𝑮𝑴𝑺 = −𝑃

    𝐵

    𝑃𝑇𝑼.𝛁𝒎 + 𝝎

    𝜕𝒎𝜕𝑝

    𝑑𝑝

    𝐿𝑣 𝑃𝐵

    𝑃𝑇𝑼.𝛁𝒒 + 𝝎

    𝜕𝒒𝜕𝑝

    𝑑𝑝

    𝑷 − 𝑬 =𝑸𝒅𝒊𝒗𝑮𝑴𝑺

    METHOD

    ENERGETICS FRAMEWORK(Neelin & Held 1987; Raymond 2009)

    3

    Net energy flux into atmosphere

    Gross Moist Stability

  • RESULTS

    GMS IS A UNIQUE FUNCTION OF

    WATER VAPOR

    4

    𝑷 − 𝑬 =𝑸𝒅𝒊𝒗𝑮𝑴𝑺

    𝑷 − 𝑬 =𝑸𝒅𝒊𝒗

    ൗ𝟖𝟎. 𝟒 𝑪𝑾𝑽 − 𝟏. 𝟑

    Jalihal et al. (2019) Nat. Comm.

  • RESULTS

    (P-E) OVER THE LAST 22,000 YRS

    5

    𝑷 − 𝑬 =𝑸𝒅𝒊𝒗

    ൗ𝟖𝟎. 𝟒 𝑪𝑾𝑽 − 𝟏. 𝟑

    Jalihal et al. (2019) Nat. Comm.

  • RESULTS

    QDIV DRIVES (P-E) DURING

    HOLOCENE

    6

    𝑷 − 𝑬 =𝑸𝒅𝒊𝒗

    ൗ𝟖𝟎. 𝟒 𝑪𝑾𝑽 − 𝟏. 𝟑

    CWV fixed at pre-industrial values.

    Jalihal et al. (2019) Nat. Comm.

  • RESULTS

    WATER VAPOR PLAYS CRUCIAL

    ROLE DURING DEGLACIAL

    7

    𝑷 − 𝑬 =𝑸𝒅𝒊𝒗

    ൗ𝟖𝟎. 𝟒 𝑪𝑾𝑽 − 𝟏. 𝟑

    Qdiv fixed at pre-industrial values.

    Jalihal et al. (2019) Nat. Comm.

  • RESULTS

    GREENHOUSE GASES AND ICE

    SHEETS AFFECT GMS ALONE

    8

    𝑷 − 𝑬 =𝑸𝒅𝒊𝒗

    ൗ𝟖𝟎. 𝟒 𝑪𝑾𝑽 − 𝟏. 𝟑GHG and ice sheets do not influence Qdiv

    Jalihal et al. (2019) Nat. Comm.

    Qdiv

    (m

    m d

    ay

    -1)

    Qdiv

    (m

    m d

    ay

    -1)

  • RESULTS

    ORBITAL FORCING AFFECTS BOTH

    GMS AND QDIV

    9

    𝑷 − 𝑬 =𝑸𝒅𝒊𝒗

    ൗ𝟖𝟎. 𝟒 𝑪𝑾𝑽 − 𝟏. 𝟑

    Even though both Qdiv and GMS are influenced, GMS is dominant, when boundary conditions are that of LGM.

    Jalihal et al. (2019) Nat. Comm.

    Qdiv

    (m

    m d

    ay

    -1)

  • Energy available

    GHG & Ice sheets

    Total column water vapor

    Surface temperature

    Precipitation

    1 2

    1 - Dominant during the Deglacial

    2 - Dominant during the Holocene

    Insolation

    Jalihal et al. (2019) Nat. Comm.

  • Long version

  • MOTIVATION

    INSOLATION OVER LAST 22,000 YRS

    1

    HoloceneDeglacial

    Summer insolation over India

  • MOTIVATION

    THIS VARIATION IS DUE TO

    PRECESSION OF EARTH

    1

    HoloceneDeglacial

    23,000 yrs

  • OBJECTIVE

    DIFFERENT SENSITIVITY OF

    MONSOON TO INSOLATION

    2

    TraCE21K simulation

    Model: CCSM3, fully coupled ESM, with transient boundary conditions,3.75ᵒ x 3.75ᵒ

    Duration: 22 Kyrs

  • OBJECTIVE

    DIFFERENT SENSITIVITY OF

    MONSOON TO INSOLATION

    2

    Deglacial forcings: Insolation greenhouse gasesice sheets

    Holocene forcings: Mainly insolation

  • OBJECTIVE

    OBJECTIVE

    Identify the feedbacks.

    Quantify the role of forcings and feedbacks.

    3

  • Method

    4

  • Based on the equations for conservation of moisture & Moist Static Energy.

    𝑃𝑡

    𝑃𝑏

    𝑈. 𝛻𝑚 + 𝜔𝜕𝑚

    𝜕𝑝𝑑𝑝 = 𝑔[𝐹𝑏 − 𝐹𝑡]

    𝑃𝑡

    𝑃𝑏

    𝑈. 𝛻𝑞 + 𝜔𝜕𝑞

    𝜕𝑝𝑑𝑝 = 𝑔[𝐸 − 𝑃]

    m - Moist Static Energy;

    (m = Cp*T + g*Z + Lv *q)

    Fb - Bottom Fluxes

    Ft - Fluxes at Top of Atm.

    u - x component of velocity

    METHOD

    ENERGETICS FRAMEWORK

    q - Specific Humidity (kg/Kg)

    ω - Vertical velocity (Pa/s)

    Pb - Surface Pressure

    Pt - Top Pressure

    v - y component of velocity

    5

  • 𝑷 − 𝑬 =𝑸𝒅𝒊𝒗𝑮𝑴𝑺

    METHOD

    ENERGETICS FRAMEWORK(Neelin & Held 1987; Raymond 2009)

    6

    𝑮𝑴𝑺 = −𝑃

    𝐵

    𝑃𝑇𝑼.𝛁𝒎+ 𝝎

    𝜕𝒎𝜕𝑝

    𝑑𝑝

    𝐿𝑣 𝑃𝐵

    𝑃𝑇𝑼.𝛁𝒒 + 𝝎

    𝜕𝒒𝜕𝑝

    𝑑𝑝

  • 𝑮𝑴𝑺 = −𝑃

    𝐵

    𝑃𝑇𝑼.𝛁𝒎 + 𝝎

    𝜕𝒎𝜕𝑝

    𝑑𝑝

    𝐿𝑣 𝑃𝐵

    𝑃𝑇𝑼.𝛁𝒒 + 𝝎

    𝜕𝒒𝜕𝑝

    𝑑𝑝

    𝑷 − 𝑬 =𝑸𝒅𝒊𝒗𝑮𝑴𝑺

    METHOD

    ENERGETICS FRAMEWORK(Neelin & Held 1987; Raymond 2009)

    6

    Net energy flux into atmosphere (top + bottom)

    Over land net surface energy fluxes are small.

  • 𝑷 − 𝑬 =𝑸𝒅𝒊𝒗𝑮𝑴𝑺

    METHOD

    ENERGETICS FRAMEWORK(Neelin & Held 1987; Raymond 2009)

    6

    m

    ω𝑮𝑴𝑺 = −

    𝑃𝐵

    𝑃𝑇𝑼.𝛁𝒎 + 𝝎

    𝜕𝒎𝜕𝑝

    𝑑𝑝

    𝐿𝑣 𝑃𝐵

    𝑃𝑇𝑼.𝛁𝒒 + 𝝎

    𝜕𝒒𝜕𝑝

    𝑑𝑝

    Gross Moist Stability.

    Primarily depends on vertical profile of m and ω

  • 𝑮𝑴𝑺 = −𝑃

    𝐵

    𝑃𝑇𝑼.𝛁𝒎 + 𝝎

    𝜕𝒎𝜕𝑝

    𝑑𝑝

    𝐿𝑣 𝑃𝐵

    𝑃𝑇𝑼.𝛁𝒒 + 𝝎

    𝜕𝒒𝜕𝑝

    𝑑𝑝

    𝑷 − 𝑬 =𝑸𝒅𝒊𝒗𝑮𝑴𝑺

    METHOD

    ENERGETICS FRAMEWORK(Neelin & Held 1987; Raymond 2009)

    6

    m

    ω

  • Qdiv = TOA_Net_SW - TOA_OLR + SFC_RAD + SHF + LHF

    TOA_Net_SW- Net Short Wave at Top of Atm

    TOA_OLR - Net Outgoing Longwave Radiation

    Qnet

    RESULTS

    A CLOSER LOOK AT QDIV

    7

    Qdiv over land is influenced by insolation and cloud radiative feedback.

  • Results

    8

  • RESULTS

    GMS IS A UNIQUE FUNCTION OF

    WATER VAPOR

    9

    Jalihal et al. (2019) Nat. Comm.

  • RESULTS

    GMS IS A UNIQUE FUNCTION OF

    WATER VAPOR

    9

    𝑷 − 𝑬 =𝑸𝒅𝒊𝒗𝑮𝑴𝑺

    𝑷 − 𝑬 =𝑸𝒅𝒊𝒗

    ൗ𝟖𝟎. 𝟒 𝑪𝑾𝑽 − 𝟏. 𝟑

    Jalihal et al. (2019) Nat. Comm.

  • RESULTS

    (P-E) OVER THE LAST 22,000 YRS

    10

    𝑷 − 𝑬 =𝑸𝒅𝒊𝒗

    ൗ𝟖𝟎. 𝟒 𝑪𝑾𝑽 − 𝟏. 𝟑

    Jalihal et al. (2019) Nat. Comm.

  • RESULTS

    QDIV DRIVES (P-E) DURING

    HOLOCENE

    10

    𝑷 − 𝑬 =𝑸𝒅𝒊𝒗

    ൗ𝟖𝟎. 𝟒 𝑪𝑾𝑽 − 𝟏. 𝟑

    CWV fixed at pre-industrial values.

    Jalihal et al. (2019) Nat. Comm.

  • RESULTS

    WATER VAPOR PLAYS CRUCIAL

    ROLE DURING DEGLACIAL

    10

    𝑷 − 𝑬 =𝑸𝒅𝒊𝒗

    ൗ𝟖𝟎. 𝟒 𝑪𝑾𝑽 − 𝟏. 𝟑

    Qdiv fixed at pre-industrial values.

    Jalihal et al. (2019) Nat. Comm.

  • Role of different forcings

    11

  • RESULTS

    GREENHOUSE GASES AFFECT GMS

    ALONE

    12

    𝑷 − 𝑬 =𝑸𝒅𝒊𝒗

    ൗ𝟖𝟎. 𝟒 𝑪𝑾𝑽 − 𝟏. 𝟑

    GHG does not influence Qdiv

    Jalihal et al. (2019) Nat. Comm.

    Qdiv

    (m

    m d

    ay

    -1)

  • RESULTS

    ICE SHEETS AFFECT GMS ALONE

    13

    𝑷 − 𝑬 =𝑸𝒅𝒊𝒗

    ൗ𝟖𝟎. 𝟒 𝑪𝑾𝑽 − 𝟏. 𝟑

    Ice sheets do not influence Qdiv

    Jalihal et al. (2019) Nat. Comm.

    Qdiv

    (m

    m d

    ay

    -1)

  • RESULTS

    ORBITAL FORCING AFFECTS BOTH

    GMS AND QDIV

    14

    𝑷 − 𝑬 =𝑸𝒅𝒊𝒗

    ൗ𝟖𝟎. 𝟒 𝑪𝑾𝑽 − 𝟏. 𝟑

    Even though both Qdiv and GMS are influenced, GMS is dominant.

    Jalihal et al. (2019) Nat. Comm.

    Qdiv

    (m

    m d

    ay

    -1)

  • RESULTS

    ORBITAL FORCING WITH GLACIAL

    BOUNDARY CONDITIONS

    15

    𝑷 − 𝑬 =𝑸𝒅𝒊𝒗

    ൗ𝟖𝟎. 𝟒 𝑪𝑾𝑽 − 𝟏. 𝟑

    ORB: orbital parameters only. Constant LGM values for all other boundary conditions.

    During cold periods, orbital forcing drives monsoon through GMS.

    Jalihal et al. (2019) Nat. Comm.

    Qdiv

    (m

    m d

    ay

    -1)

  • Energy available

    Precipitation

    1 2

    Insolation

    GMS

    1 - Dominant during the Deglacial

    2 - Dominant during the Holocene

    Jalihal et al. (2019) Nat. Comm.

  • Energy available

    GHG & Ice sheets

    Precipitation

    1 2

    1 - Dominant during the Deglacial

    2 - Dominant during the Holocene

    Insolation

    GMS

    Jalihal et al. (2019) Nat. Comm.

  • Energy available

    GHG & Ice sheets

    Total column water vapor

    Surface temperature

    Precipitation

    1 2

    1 - Dominant during the Deglacial

    2 - Dominant during the Holocene

    Insolation

    Jalihal et al. (2019) Nat. Comm.

  • Conclusions

    19

  • CONCLUSIONS

    CONCLUSIONS

    • Changes in insolation is an initial trigger, final response involves feedbacks as well.

    • Water vapor feedback amplifies solar forcing during deglacial.

    • Cloud radiative feedback influences monsoon during Holocene.

    20

  • CONCLUSIONS

    CONCLUSIONS

    • Insolation can drive monsoon through two different pathways.

    • Greenhouse gases and ice sheets only affect GMS.

    20

    • Through energy available during warm periods, and through GMS during cold periods

  • Thank you

    21

  • Extra Slides

    22

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