NASA’s Spaceflight Visual Impairment Intracranial Pressure (VIIP) Risk: Clinical Correlations & Pathophysiology Bill Tarver, M.D. Deputy Chief & Medical Director, NASA Clinical Services Branch & Christian Otto, M.D. VIIP Lead Scientist Aerospace Medicine Grand Rounds Page No. 1 May 22, 2012 USRA Houston, TX Visual Impairment Intracranial Pressure Risk Working Risk Statement: • "Given that the microgravity environment causes cepahld fluid shift in astronauts, there is a high probability that all astronauts have intracranial hypertension (IHT) to some degree. Presently these symptoms have manifested themselves as changes in eye structure such as papilledema, globe flattening, choroidal folds, cotton wool spots (CWS) increased retinal nerve fiber layer and/or decreased near vision, along with post mission spinal opening pressures ranging between 21 - 28.5 cmH20 for symptomatic astronauts. If the IHT is not treated, there is a risk of damage to the optic nerve and possible reduced vision capability long term.” Page No. 2 Clinical Data Overview: flight Changes in Vision %( 7%996 5*4Q&6( 9)( - 6- 7+= *. G- In 79*<+ %DRRC; 96 9' %)( 9%( . %. - 7%4H7 9*&' % . C7)(Active >+%@)7)6( J B F546(population 9E%( 7%7HPE% ( 7%7 :% *9- 4%D( 9) 4%:+%&9)6( C astronaut mean age=47y 7A Majority are presbyopic +%*4J B 546( 9E%( 7%7 8 )9' 9)( 9%. J B 546( 9E%( 7%7A $)( 97 6::%4%. )( &+- . % 80% wear vision correction (32% contact lenses) way' to “slider” 696& 46?adjust )&+%( the 7%7 *4%*+ 76 *@*)+*<+%A D( - +94* Incorrect 7+)? FE%( 7 way " *7%H C8adjust ' )&' the “slider” to From postflight questionnaires (1989 - 2011): ' %9)( 9%. 546( 9E%( 7%7*4%)( - 7%C)7 ; 46@). %. 8 )9' %@%4= ; *)46: $4- 56&*+7 ) %'and , "$ 50% = of long- duration (ISS) position• 25% of short-duration (Shuttle) mission astronauts report a subjective degradation in vision ! " # $%&' ( )&*+, - ). %/ 011123 “Space Anticipation Glasses” ed to adjust the Slider (blue arrow in picture below) for clearer vision, indica ! " # $%&' ( to the right (approximately)... p position No. 3 Superfocus glasses and slider in the full left stop position, position aringPagethe Common Characteristics of the Cases • Approximately 6 month duration ISS mission • All had normal preflight eye examinations • Past medical history was negative for systemic disease; and none had used medications before or during their mission that could increase ICP (e.g., vitamin A, tetracycline, corticosteroids, or nalidixic acid) Page No. 4 Common Characteristics • None experienced losses in best-corrected visual acuity, color vision or stereopsis • ISS cabin pressure, and oxygen were at normal operating levels. • Elevations in CO2 Page No. 5 Pre & Post Flight Papilledema [Top Pre Flight] Fundoscopic images of the right and left optic disc. [Bottom Post Flight] Fundoscopic images of the right and left optic disc showing Grade 3 edema at the right optic disc and Grade 1 edema at the left optic disc. Page No. 6 Pre Flight OD OS Post Flight OD OS Choroidal Folds Postflight Postflight OD OD Preflight Inferior Page No. 7 OS Superior Postflight Inferior Superior In Flight B-scan Ultrasound Page No. 8 Mean ONSD Measurement & ICP Because of a variable pressure-diameter relationship, the clinical relevance of this method relies on the demonstration of ongoing enlargement on serial US studies. Clinically ONSD 5.9mm=20mmHg Page No. 9 Increased Optic Nerve Sheath Diameter On-Orbit OS OD 12 mm Page No. 10 MRI Globe Imaging T1 MRI orbital imaging of the right eye. Pre flight (left) and Post flight (right) showing flattening of the posterior globe. Page No. 11 Flattening of Posterior Wall – and Raised Optic Disk Elevation of optic disc Page No. 12 CONFIDENTIAL Pre & Post Flight Testing MRI 2D Ultrasound L-12/9m and L-6/3m L-21/18m R+1/3d R+1/3d Combined with training 3T or better using specific ocular imaging protocols Vision Exam Page No. 13 • Fundoscopy • Tonometry • OCT In Flight: L+30 Days & R-30 Days Vision Exam (includes L+100d) Fundoscopy Tonometry 2D Ultrasound Page No. 14 Clinical Practice Guideline for SpaceflightInduced Intracranial Hypertension Page No. 15 VIIP Clinical Practice Guideline & Case Definition Case Classification (U.S. ISS Crew) (As of Jan 2012) 36 U.S. ISS crew flown to date: • Confirmed non-cases N=2 • Unclassified crew N=19 • CPG Class One N=2 • CPG Class Two N=8 • CPG Class Three N=1 • CPG Class Four N=4 N Confirmed Non Cases • • Page No. 16 < .50 diopter cycloplegic refractive change No evidence of papilledema, nerve sheath distention, choroidal folds, globe flattening, scotoma or cotton wool spots compared to baseline. 2 VIIP Clinical Practice Guideline & Case Definition Case Classification (U.S. ISS Crew) (As of Jan 2012) Un-Classified Crew • • Too little evidence at present for definitive classification Early ISS flyers with no, or limited testing Class 1 (repeat OCT and visual acuity in 6 weeks) • • • Case Class 19 2 ≥ .50 diopter cycloplegic refractive change and/or cotton wool spot No evidence of papilledema, nerve sheath distention, choroidal folds, globe flattening, scotoma compared to baseline. CSF opening pressure (if measured) ≤ 25 cmH2O Class 2 (repeat OCT, cycloplegic refraction, fundus exam and threshold visual field every 4 -6 weeks x 6 months, repeat MRI in 6 months) 2/10 • ≥ .50 diopter cycloplegic refractive changes or cotton wool spot • Choroidal folds and/or optic nerve sheath distension and/or globe flattening and/or scotoma • No evidence of papilledema • CSF opening pressure ≤ 25 cm H2O (if measured) 8 17 Page No. 17 VIIP Clinical Practice Guideline & Case Definition Case Classification (U.S. ISS Crew) (As of Jan 2012) Case Class Class 3 (repeat OCT, cycloplegic refraction, fundus exam and threshold visual field every 4 -6 weeks x 6 months, repeat MRI in 6 months) • • • • ≥ .50 diopter cycloplegic refractive changes and/or cotton wool spot Optic nerve sheath distension, and/or globe flattening and/or choroidal folds and/or scotoma Papilledema of Grade 0-2. CSF opening pressure ≤ 25 cm H2O Class 4 (institute treatment protocol as per CPG) • • • • • 1 4 ≥ .50 diopter cycloplegic refractive changes and/or cotton wool spot Optic nerve sheath distension, and/or globe flattening and/or choroidal folds and/or scotoma Papilledema Grade 2 or above. Presenting symptoms of new headache, pulsatile tinnitus and/or transient visual obscurations CSF opening pressure >25 cm H2O 18 Page No. 18 Impact of Inflight Exacerbating Factors? Resistive Exercise Does in-flight resistance training cause additional transient elevations in ICP? High Oral Sodium Intake Prepackaged Foods High in sodium Up to 5000mg+ per day Inflight Pharmaceuticals Effects on VIIP? Page No. 19 CO2 Levels on ISS Pressure Adapted from Alperin et al. Radiology, 2000 CO2 is an extremely potent vasodilator • Every 1mmHg increase PaCO2=4% increase in dilation • Cerebral blood vessels are already congested CO2 X X CO2 mission average=3.56mmHg (0.33%) • 10x normal sea level atmospheric: 0.0314% • Average Peak CO2=8.32mmHg (0.7%) (20x) CO2 also causes increased CSF production Page No. 20 Cephalad Fluid Shift Piecing Together Visual Impairment and Elevated Intracranial Pressure in Spaceflight Currently-A Three-Part Story 1. The Vascular System + Page No. 21 3. The Eye 2. The Brain + A Working Model: Potential Interaction of the CNS, Vascular, & Ocular System in Microgavity Interstitial Edema +ICP +OCSFP Cerebral Venous Blood +CSFP +OVP +VP X 9.8m/s2 Loss of Hydrostatic Drainage Adapted from Rekate Page No. 22 Vascular Capacitance (dV/dP): Venous & Arterial 20%=1L Page No. 23 70-80%=4L Correlation of BMI with ICP in 71 Non-IIH Subjects • • Mean age 45.7±11.3 Mean BMI 23.7±2.7 kg/m2 (17.3–29.4) CSF-P correlated with: • Higher BMI (P<0.001; r=0.50) • Higher systolic blood pressure (P=0.04; r=0.24), • Higher intraocular pressure (P<0.001; r=0.76) Ren et. al. Cerebrospinal fluid pressure correlated with body mass index. Arch Clin Exp Ophthalmol. July 2011 Page No. 24 Why Does Elevated Blood Pressure and Increased Resistance Matter? Page No. 25 Decreased Venous Compliance and Elevated CVP in Hypertensives "central venous pressure" A major determinant of preload Normal CVP=2-6mmHg A change in CVP is determined by the change in volume (ΔV) of blood within the thoracic veins divided by the compliance of the these veins according to the following equation: ΔCVP = ΔV / Cv CVP, measured in patients with essential hypertension is modestly increased, even in the absence of congestive heart failure i.e. normal pumping ability of the heart Decreased venous compliance contributes to the increase in CVP in hypertensive patients • • • Olivari et al. Pulmonary hemodynamics and right ventricular function in hypertension. Circulation 1978;57:1185-1190 Safar et al. Venous system in essential hypertension. Clin Science 1985 Nov;69(5):497-504. London et al. Hemodynamic effects of head-down tilt in normal subjects and sustained hypertensive patients Am J Physiol Heart Circ Physiol August 1, 1983 245:(2) H194-H202 Page No. 26 LV Hypertrophy LV Strain 3mmHg 6mmHg CVP in Normotensives vs Hypertensives During 10o HDT Higher increase in cardiac output in hypertensive patients due to a higher change in CVP related to decreased venous distensibility A decrease in venous vascular resistance during tilt among normotensives: due to inhibition of vasoconstrictor tone (-SNS +PNS). This led to partial relief of the congestion; minimizing the effects of blood volume distribution. Hypertensives did not demonstrate a decrease in venous tone The absence of this buffering effect of the veins in the hypertensives may be responsible for the higher CVP and CO. Page No. 27 N=9 N=7 London et al. 1983. Hemodynamic effects of head-down tilt in normal subjects and sustained hypertensive patients. Am J Physiol. Factors Increasing Venous Tone will Increase Cerebral Venous Outflow Resistance Resting Tone of Venous Vessels Influenced by: • (CVP) SNS tone↑ Resting Blood Pressure • Endothelin↑ • Nitric oxide↓ • Inflammatory cytokines ↑ Baseline Stiffness of Arterial Vessels Influenced by: • Serum lipids • Serum glucose • Homocysteine levels • Aerobic fitness & vessel wall stiffness • Nitric oxide levels Page No. 28 Although effects of tone less on venous side vs arterial, volume is much greater Med Ops/Research Occupational Data Mining ISS Crew: Cardiovascular Variables Data Mining Variable Significant Correlation with CPG Biochemistry: LDL √ HDL - Triglycerides - Hemoglobin A1c √ Fasting serum glucose √ Homocysteine √ Body Composition: Body Mass Index √ Percentage Body Fat √ Cardiac: Resting blood pressure (pre-in-post flight) √ Pulse Pressure (pre-in-post flight) √ CT Coronary Calcium Score - Aerobic Capacity: Page No. 29 Low Maximal Oxygen Uptake √ All correlated factors adversely affect vascular structure & function Loss of Hydrostatic Drainage, Fluid Shift, & Cerebral Venous Congestion 1G 0G 1G Supine CEPHALAD FLUID SHIFT X 9.8m/s2 Loss of Hydrostatic Drainage Adapted from Rowell, 1988 Adapted from Hargens & Richardson, Respiratory Physiology & Neurobiology. 2009 Page No. 30 Tilt Angle vs ICP & CVP: Positional Fluid Shifts ICP 24mmHg CVP=9mmHg ICP 9.2mmHg CVP=5mmHg ICP-2.3mmHg CVP=0mmHg 1. Chapman et al. The Relationship between Ventricular Fluid Pressure and Body Position in Normal Subjects with Shunts. Neurosurgery 1990 2. Hemodynamic changes due to Trendelenburg positioning and pneumoperitoneum during laproscopic hysterectomy, Acta Anaesthesiologica Scandiavica. 1995 Page No. 31 Redistribution of Venous Pressures From 1G to 0G ICP = CSFout resistance x CSFformation + SSSpressure 0G Standing 1G -2 15-20 7-9 9.8m/s2 Cranium is rigid Venous congestion Obligate arterial flow Transcapillary leak ++ICP~30-40 X 1. Hirvonen et al. Hemodynamic changes due to Trendelenburg positioning and pneumoperitoneum during laproscopic hysterectomy, Acta Anaesthesiologica Scandiavica. 1995 2. Hinghofer-Szalkay Gravity, the hydrorostatic indifference concept and the cardiovascular system. European Journal of Applied Physiology, 2010 Page No. 32 3. Chapman et al. The Relationship between Ventricular Fluid Pressure and Body Position in Normal Subjects with Shunts. Neurosurgery 1990 4. Gisolf et al. Human cerebral outflow pathway depends on posture and central venous pressure. Journal of Physiology, 2004. In Flight B-scan Ultrasound Page No. 33 MRI Globe Imaging T1 MRI orbital imaging of the right eye. Pre flight (left) and Post flight (right) showing flattening of the posterior globe. Page No. 34 MRI Signs of Elevated ICP: IIH vs VIIP MRI Signs of Elevated ICP: IIH vs VIIP Imaging Assessment Present in IIH (Specificity) Seen in VIIP Flattening of Posterior Globes 100% Yes Optic Nerve Protrusion 100% Yes Optic Nerve Sheath Distension 88.4% Yes Optic Nerve Tortuosity 86% Yes Maralani et al. Accuracy of brain imaging in the diagnosis of idiopathic intracranial hypertension. Clinical Radiology. Dec. 2011. Page No. 35 Key Brain Areas CSF Resorbtion Interstitial fluid CSF Production Cranial Volume = Brain + CSF + Blood Page No. 36 (AG-Venous/Lymphatic) Venous Congestion Normal CSF Diffusion Gradient Normal SSVP:CSFP= 0.60 Therefore delta driving pressure only~3-5mmHg Venous Sinus Pressure=5-7mmHg ICP= 10mmHg Page No. 37 The Brain as an Expansile Vascular Organ Within a Rigid Cranium Page No. 38 Venous Congestion causes Increased Transcapillary Pressure & Decreased Absorbtion X Interstitial edema Page No. 39 ↑Venous Pressure Dural Venous Transverse Sinus Page No. 40 Expanding Brain Parenchyma & Cerebellum Compresses Transverse Sinus Page No. 41 MRI Venography of Stenosed Right Transverse Sigmoid Sinus Page No. 42 Reversibility of Venous Sinus Obstruction with Reduction of CSF Pressure A. ICP 50cmH20 Bilateral Stenosis Transverse Sinus B. After Lumbar Puncture removal of CSF x2 with resultant reduction in ICP C. Placement of Ventriculoperitoneal Shunt for continuous CSF drainage and ICP reduction Page No. 43 CSF Production: Choroid Plexus Choroid plexus in lateral, third & fourth ventricle produces 70-90% of CSF in brain Increased filtration? Page No. 44 Choroidal Cell Responses in MicrogravityAquaporin-1 Expression Ground Control 1G Normal Control Choroid Cell 0G & Hind Limb Abnormal 0G Analog Choroid Cell Page No. 45 Gabrion et al. Choroidal responses in microgravity. Acta Astronautica. 1995 Immunodetection of AQP1 (in green) at the apical pole of choroid plexus, (A) control rat (homogeneously covered with long bulbous apical microvilli, and tufts of kinocillia) (C) model simulating cephalad fluid shift. AQP1 was reduced 64% after 14d spaceflight (STS-58), by 44% after 14 days HLU, and by 68% after 28d HLU. A net decrease was noted, suggesting CSF production was decreased. Loss of microvilli, failure of exocytosis, loss of kinocillia Suggests brain adaptation in microgravity with a reduction in CSF secretory activity. Rat CP After 14 days in Microgravity Scanning Electron Micrograph Rat Choroidal Cell -Lateral Ventricle Transmission Electron Micrograph Rat Choroidal CellApical Pole Microvilli Abnormalities • Is there a set-point for elevated ICP that triggers a down-regulation of aquaporin 1 expression? • AQP1 Knockout mice had 20-25% reduction in CSF production (Oshio et al 2005) • Recent data from hydrocephalic rats (elevated ICP) shows a significant down regulation of AQP1 in in choroid plexus (Paul et al. 2009) • Hyrdocephalus seems to be associated with AQP1 downregulation in the choroid plexus which could be an adaptive mechanism to reduce CSF production and ICP Page No. 46 Pre & Post Flight Papilledema [Top Pre Flight] Fundoscopic images of the right and left optic disc. [Bottom Post Flight] Fundoscopic images of the right and left optic disc showing Grade 3 edema at the right optic disc and Grade 1 edema at the left optic disc. Page No. 47 Pre Flight OD OS Post Flight OD OS The Lamina Cribosa: Barrier Between the Intraocular Space and SAS The LC serves as a barrier to separate the intraorbital space, with typically higher pressure, from the subarachnopid space, with typically lower pressure. The LC therefore prevents orbital contents from leaking into the subarachnoid space Page No. 48 Lamina Cribosa Structure • • • • LC is a series of cribiform plates, with pores that line up to permit nerve axons to pass through Average adult: 1.2 million axons pass through the lamina cribrosa in approx 250 nerve bundles All of these axons depend on slow and fast axoplasmic transport for viability and synapses production LC cores are filled with fibrillar collagen and elastic fibres, during aging these constituents are altered Page No. 49 TLP Differences & Visual Field Defect 12.5 6.6 1.4 Control group Normal Pressure Glaucoma High Pressure Glaucoma The extent of glaucomatous visual field loss was negatively correlated with the height of the CSF-P [as CSFp went down vis field loss increased] and positively correlated with the TLP difference [as tlp increased, visual field loss increased]. Page No. 50 Amount of glaucomatous visual field defect correlated positively with the TLP pressure difference (P _ 0.005) r=0.69 Ren et al. 2009. Cerebrospinal Fluid Pressure in Glaucoma Choroidal Folds Postflight Postflight OD OD OS Preflight Inferior Page No. 51 Postflight Superior Inferior Superior Venous Congestion & Elevated ICP: Transmitted to the Choroid? Ansari et al. 2003. Measurement of Choroidal blood flow in Zero Gravity KC135 parabolic flight experiment. • Choroidal volume and flow increase significantly in low G environment when compared with the baseline data (1G): 75% increase for volume, and 105% for flow. P Transmitted via the ophthalmic veins P P Venous Sinus Page No. 52 MRI Brain Venogram Next Steps MRI/MRV analysis Multivariate analysis of Cardio/CNS & ocular variables • As “N” grows sensitivity of multivariate analysis increases • Addition of IP “cases and non-cases will increase “N” 33% Data review for dose response effect Data collection from Inflight Ocular study Inflight ocular study Vittamed 205 Malm Pilot in Umea 6 NRAs awarded • 3 Inflight (Stenger/Dulchavsky/Hargens) • 1 Imaging (Roberts) • 2 Non Invasive ICP (Detinger/Williams) Countermeasure evaluation Page No. 53 NASA’s Spaceflight Visual Impairment Intracranial Pressure (VIIP) Risk: Clinical Correlations & Pathophysiology Bill Tarver, M.D. Deputy Chief & Medical Director, NASA Clinical Services Branch & Christian Otto, M.D. VIIP Lead Scientist Aerospace Medicine Grand Rounds Page No. 54 May 22, 2012 USRA Houston, TX